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1. EUSO-SPB1 Mission and Science

Author: Collaboration, JEM-EUSO, Abdellaoui, G., Abe, S., Adams. Jr., J. H., Allard, D., Alonso, G., Anchordoqui, L., Anzalone, A., Arnone, E., Asano, K., Attallah, R., Attoui, H., Pernas, M. Ave, Bachmann, R., Bacholle, S., Bagheri, M., Bakiri, M., Baláz, J., Barghini, D., Bartocci, S., Battisti, M., Bayer, J., Beldjilali, B., Belenguer, T., Belkhalfa, N., Bellotti, R., Belov, A. A., Benmessai, K., Bertaina, M., Bertone, P. F., Biermann, P. L., Bisconti, F., Blaksley, C., Blanc, N., Blin-Bondil, S., Bobik, P., Bogomilov, M., Bolmgren, K., Bozzo, E., Briz, S., Bruno, A., Caballero, K. S., Cafagna, F., Cambié, G., Campana, D., Capdevielle, J. N., Capel, F., Caramete, A., Caramete, L., Caruso, R., Casolino, M., Cassardo, C., Castellina, A., Catalano, O., Cellino, A., Černý, K., Chikawa, M., Chiritoi, G., Christl, M. J., Colalillo, R., Conti, L., Cotto, G., Crawford, H. J., Cremonini, R., Creusot, A., Cummings, A., Gónzalez, A. de Castro, de la Taille, C., del Peral, L., Desiato, J., Damian, A. Diaz, Diesing, R., Dinaucourt, P., Djakonow, A., Djemil, T., Ebersoldt, A., Ebisuzaki, T., Eser, J., Fenu, F., Fernández-González, S., Ferrarese, S., Filippatos, G., Finch, W., Fornaro, C., Fouka, M., Franceschi, A., Franchini, S., Fuglesang, C., Fujii, T., Fukushima, M., Galeotti, P., García-Ortega, E., Gardiol, D., Garipov, G. K., Gascón, E., Gazda, E., Genci, J., Golzio, A., Gorodetzky, P., Gregg, R., Green, A., Guarino, F., Guépin, C., Guzmán, A., Hachisu, Y., Haungs, A., Heigbes, T., Carretero, J. Hernández, Hulett, L., Ikeda, D., Inoue, N., Inoue, S., Isgrò, F., Itow, Y., Jammer, T., Jeong, S., Jochum, J., Joven, E., Judd, E. G., Jung, A., Kajino, F., Kajino, T., Kalli, S., Kaneko, I., Kasztelan, M., Katahira, K., Kawai, K., Kawasaki, Y., Kedadra, A., Khales, H., Khrenov, B. A., Kim, Jeong-Sook, Kim, Soon-Wook, Kleifges, M., Klimov, P. A., Kreykenbohm, I., Krizmanic, J. F., Królik, K., Kungel, V., Kurihara, Y., Kusenko, A., Kuznetsov, E., Lahmar, H., Lakhdari, F., Licandro, J., Campano, L. López, Martínez, F. López, Mackovjak, S., Mahdi, M., Mandát, D., Manfrin, M., Marcelli, L., Marcos, J. L., Marszał, W., Martín, Y., Martinez, O., Mase, K., Mastafa, M., Matthews, J. N., Mebarki, N., Medina-Tanco, G., Menshikov, A., Merino, A., Mese, M., Meseguer, J., Meyer, S. S., Mimouni, J., Miyamoto, H., Mizumoto, Y., Monaco, A., Ríos, J. A. Morales de los, Nachtman, J. M., Nagataki, S., Naitamor, S., Napolitano, T., Neronov, A., Nomoto, K., Nonaka, T., Ogawa, T., Ogio, S., Ohmori, H., Olinto, A. V., Onel, Y., Osteria, G., Otte, A. N., Pagliaro, A., Painter, W., Panasyuk, M. I., Panico, B., Parizot, E., Park, I. H., Pastircak, B., Paul, T., Pech, M., Pérez-Grande, I., Perfetto, F., Peter, T., Picozza, P., Pindado, S., Piotrowski, L. W., Piraino, S., Plebaniak, Z., Pollini, A., Popescu, E. M., Prevete, R., Prévôt, G., Prieto, H., Przybylak, M., Puehlhofer, G., Putis, M., Reardon, P., Reno, M. H., Reyes, M., Ricci, M., Frías, M. D. Rodríguez, Matamala, O. F. Romero, Ronga, F., Sabau, M. D., Saccá, G., Sagawa, H., Sahnoune, Z., Saito, A., Sakaki, N., Salazar, H., Sánchez, J. L., Balanzar, J. C. Sanchez, Santangelo, A., Sanz-Andrés, A., Saprykin, O. A., Sarazin, F., Sato, M., Scagliola, A., Schanz, T., Schieler, H., Schovánek, P., Scotti, V., Serra, M., Sharakin, S. A., Shimizu, H. M., Shinozaki, K., Soriano, J. F., Sotgiu, A., Stan, I., Strharský, I., Sugiyama, N., Supanitsky, D., Suzuki, M., Szabelski, J., Tajima, N., Tajima, T., Takahashi, Y., Takeda, M., Takizawa, Y., Talai, M. C., Tameda, Y., Tenzer, C., Thomas, S. B., Tibolla, O., Tkachev, L. G., Tomida, T., Tone, N., Toscano, S., Traïche, M., Tsunesada, Y., Tsuno, K., Turriziani, S., Uchihori, Y., Valdés-Galicia, J. F., Vallania, P., Valore, L., Vankova-Kirilova, G., Venters, T. M., Vigorito, C., Villaseñor, L., Vlcek, B., von Ballmoos, P., Vrabel, M., Wada, S., Watanabe, J., Watts. Jr., J., Muñoz, R. Weigand, Weindl, A., Wiencke, L., Wille, M., Wilms, J., Yamamoto, T., Yang, J., Yano, H., Yashin, I. V., Yonetoku, D., Yoshida, S., Young, R., Zgura, I. S., Zotov, M. Yu., and Marchi, A. Zuccaro
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena
Abstract: The Extreme Universe Space Observatory on a Super Pressure Balloon 1 (EUSO-SPB1) was launched in 2017 April from Wanaka, New Zealand. The plan of this mission of opportunity on a NASA super pressure balloon test flight was to circle the southern hemisphere. The primary scientific goal was to make the first observations of ultra-high-energy cosmic-ray extensive air showers (EASs) by looking down on the atmosphere with an ultraviolet (UV) fluorescence telescope from suborbital altitude (33~km). After 12~days and 4~hours aloft, the flight was terminated prematurely in the Pacific Ocean. Before the flight, the instrument was tested extensively in the West Desert of Utah, USA, with UV point sources and lasers. The test results indicated that the instrument had sensitivity to EASs of approximately 3 EeV. Simulations of the telescope system, telescope on time, and realized flight trajectory predicted an observation of about 1 event assuming clear sky conditions. The effects of high clouds were estimated to reduce this value by approximately a factor of 2. A manual search and a machine-learning-based search did not find any EAS signals in these data. Here we review the EUSO-SPB1 instrument and flight and the EAS search., Comment: 18 pages, 19 figures
Published: 2024
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2. Reconstruction of total solar irradiance variability as simultaneously apparent from Solar Orbiter and Solar Dynamics Observatory

Author: Yeo, K. L., Krivova, N. A., Solanki, S. K., Hirzberger, J., Suárez, D. Orozco, Albert, K., Jorge, N. Albelo, Appourchaux, T., Alvarez-Herrero, A., Rodríguez, J. Blanco, Gandorfer, A., Gutierrez-Marques, P., Kahil, F., Kolleck, M., Iniesta, J. C. del Toro, Volkmer, R., Woch, J., Fiethe, B., Pérez-Grande, I., Kilders, E. Sanchis, Jiménez, M. Balaguer, Rubio, L. R. Bellot, Calchetti, D., Carmona, M., Feller, A., Fernandez-Rico, G., Fernández-Medina, A., Parejo, P. García, Blesa, J. L. Gasent, Gizon, L., Grauf, B., Heerlein, K., Korpi-Lagg, A., Maue, T., Meller, R., Vacas, A. Moreno, Müller, R., Nakai, E., Schmidt, W., Schou, J., Sinjan, J., Staub, J., Strecker, H., Torralbo, I., and Valori, G.
Subjects: Astrophysics - Solar and Stellar Astrophysics
Abstract: Solar irradiance variability has been monitored almost exclusively from the Earth's perspective. {We present a method to combine the unprecedented observations of the photospheric magnetic field and continuum intensity from outside the Sun-Earth line, which is being recorded by the Polarimetric and Helioseismic Imager on board the Solar Orbiter mission (SO/PHI), with solar observations recorded from the Earth's perspective to examine the solar irradiance variability from both perspectives simultaneously.} Taking SO/PHI magnetograms and continuum intensity images from the cruise phase of the Solar Orbiter mission and concurrent observations from the Helioseismic and Magnetic Imager onboard the Solar Dynamics Observatory (SDO/HMI) as input into the SATIRE-S model, we successfully reconstructed the total solar irradiance variability as apparent from both perspectives. In later stages of the SO mission, the orbital plane will tilt in such a way as to bring the spacecraft away from the ecliptic to heliographic latitudes of up to $33^{\circ}$. The current study sets the template for the reconstruction of solar irradiance variability as seen from outside the ecliptic from data that SO/PHI is expected to collect from such positions. {Such a reconstruction will be beneficial to factoring inclination into how the brightness variations of the Sun compare to those of other cool stars, whose rotation axes are randomly inclined.
Published: 2023
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3. Coronal voids and their magnetic nature

Author: Nölke, J. D., Solanki, S. K., Hirzberger, J., Peter, H., Chitta, L. P., Kahil, F., Valori, G., Wiegelmann, T., Suárez, D. Orozco, Albert, K., Jorge, N. Albelo, Appourchaux, T., Alvarez-Herrero, A., Rodríguez, J. Blanco, Gandorfer, A., Germerott, D., Guerrero, L., Gutierrez-Marques, P., Kolleck, M., Iniesta, J. C. del Toro, Volkmer, R., Woch, J., Fiethe, B., Cama, J. M. Gómez, Pérez-Grande, I., Kilders, E. Sanchis, Jiménez, M. Balaguer, Rubio, L. R. Bellot, Calchetti, D., Carmona, M., Deutsch, W., Feller, A., Fernandez-Rico, G., Fernández-Medina, A., Parejo, P. García, Blesa, J. L. Gasent, Gizon, L., Grauf, B., Heerlein, K., Korpi-Lagg, A., Lange, T., Jiménez, A. López, Maue, T., Meller, R., Vacas, A. Moreno, Müller, R., Nakai, E., Schmidt, W., Schou, J., Schühle, U., Sinjan, J., Staub, J., Strecker, H., Torralbo, I., Berghmans, D., Kraaikamp, E., Rodriguez, L., Verbeeck, C., Zhukov, A. N., Auchere, F., Buchlin, E., Parenti, S., Janvier, M., Barczynski, K., Harra, L., Schwanitz, C., Cuadrado, R. Aznar, Mandal, S., Teriaca, L., Long, D., and Smith, P.
Subjects: Astrophysics - Solar and Stellar Astrophysics
Abstract: Extreme ultraviolet (EUV) observations of the quiet solar atmosphere reveal extended regions of weak emission compared to the ambient quiescent corona. The magnetic nature of these coronal features is not well understood. We study the magnetic properties of the weakly emitting extended regions, which we name coronal voids. In particular, we aim to understand whether these voids result from a reduced heat input into the corona or if they are associated with mainly unipolar and possibly open magnetic fields, similar to coronal holes. We defined the coronal voids via an intensity threshold of 75% of the mean quiet-Sun (QS) EUV intensity observed by the high-resolution EUV channel (HRIEUV) of the Extreme Ultraviolet Imager on Solar Orbiter. The line-of-sight magnetograms of the same solar region recorded by the High Resolution Telescope of the Polarimetric and Helioseismic Imager allowed us to compare the photospheric magnetic field beneath the coronal voids with that in other parts of the QS. The coronal voids studied here range in size from a few granules to a few supergranules and on average exhibit a reduced intensity of 67% of the mean value of the entire field of view. The magnetic flux density in the photosphere below the voids is 76% (or more) lower than in the surrounding QS. Specifically, the coronal voids show much weaker or no network structures. The detected flux imbalances fall in the range of imbalances found in QS areas of the same size. Conclusions. We conclude that coronal voids form because of locally reduced heating of the corona due to reduced magnetic flux density in the photosphere. This makes them a distinct class of (dark) structure, different from coronal holes., Comment: 10 pages, 11 figures
Published: 2023
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4. Intensity contrast of solar network and faculae close to the solar limb, observed from two vantage points

Author: Albert, K., Krivova, N. A., Hirzberger, J., Solanki, S. K., Vacas, A. Moreno, Suárez, D. Orozco, Jorge, N. Albelo, Appourchaux, T., Alvarez-Herrero, A., Rodríguez, J. Blanco, Gandorfer, A., Gutierrez-Marques, P., Kahil, F., Kolleck, M., Volkmer, R., Iniesta, J. C. del Toro, Woch, J., Fiethe, B., Pérez-Grande, I., Kilders, E. Sanchis, Jiménez, M. Balaguer, Rubio, L. R. Bellot, Calchetti, D., Carmona, M., Feller, A., Fernandez-Rico, G., Fernández-Medina, A., Parejo, P. García, Blesa, J. L. Gasent, Gizon, L., Grauf, B., Heerlein, K., Korpi-Lagg, A., Lange, T., Jiménez, A. López, Maue, T., Meller, R., Müller, R., Nakai, E., Schmidt, W., Schou, J., Sinjan, J., Staub, J., Strecker, H., Torralbo, I., and Valori, G.
Subjects: Astrophysics - Solar and Stellar Astrophysics
Abstract: The brightness of faculae and network depends on the angle at which they are observed and the magnetic flux density. Close to the limb, assessment of this relationship has until now been hindered by the increasingly lower signal in magnetograms. This preliminary study aims at highlighting the potential of using simultaneous observations from different vantage points to better determine the properties of faculae close to the limb. We use data from the Solar Orbiter/Polarimetric and Helioseismic Imager (SO/PHI), and the Solar Dynamics Observatory/Helioseismic and Magnetic Imager (SDO/HMI), recorded at $\sim60^\circ$ angular separation of their lines of sight at the Sun. We use continuum intensity observed close to the limb by SO/PHI and complement it with the co-observed $B_{\rm LOS}$ from SDO/HMI, originating closer to disc centre (as seen by SDO/HMI), thus avoiding the degradation of the magnetic field signal near the limb. We derived the dependence of facular brightness in the continuum on disc position and magnetic flux density from the combined observations of SO/PHI and SDO/HMI. Compared with a single point of view, we were able to obtain contrast values reaching closer to the limb and to lower field strengths. We find the general dependence of the limb distance at which the contrast is maximum on the flux density to be at large in line with single viewpoint observations, in that the higher the flux density is, the closer the turning point lies to the limb. There is a tendency, however, for the maximum to be reached closer to the limb when determined from two vantage points. We note that due to the preliminary nature of this study, these results must be taken with caution. Our analysis shows that studies involving two viewpoints can significantly improve the detection of faculae near the solar limb and the determination of their brightness contrast relative to the quiet Sun.
Published: 2023
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5. Stereoscopic disambiguation of vector magnetograms: first applications to SO/PHI-HRT data

Author: Valori, G., Calchetti, D., Vacas, A. Moreno, Pariat, É., Solanki, S. K., Löschl, P., Hirzberger, J., Parenti, S., Albert, K., Jorge, N. Albelo, Álvarez-Herrero, A., Appourchaux, T., Rubio, L. R. Bellot, Rodríguez, J. Blanco, Campos-Jara, A., Feller, A., Gandorfer, A., Parejo, P. García, Germerott, D., Gizon, L., Cama, J. M. Gómez, Guerrero, L., Gutierrez-Marques, P., Kahil, F., Kolleck, M., Korpi-Lagg, A., Suárez, D. Orozco, Pérez-Grande, I., Kilders, E. Sanchis, Schou, J., Schühle, U., Sinjan, J., Staub, J., Strecker, H., Iniesta, J. C. del Toro, Volkmer, R., and Woch, J.
Subjects: Astrophysics - Solar and Stellar Astrophysics
Abstract: Spectropolarimetric reconstructions of the photospheric vector magnetic field are intrinsically limited by the 180$^\circ$-ambiguity in the orientation of the transverse component. So far, the removal of such an ambiguity has required assumptions about the properties of the photospheric field, which makes disambiguation methods model-dependent. The basic idea is that the unambiguous line-of-sight component of the field measured from one vantage point will generally have a non-zero projection on the ambiguous transverse component measured by the second telescope, thereby determining the ``true'' orientation of the transverse field. Such an idea was developed and implemented in the Stereoscopic Disambiguation Method (SDM), which was recently tested using numerical simulations. In this work we present a first application of the SDM to data obtained by the High Resolution Telescope (HRT) onboard Solar Orbiter during the March 2022 campaign, when the angle with Earth was 27 degrees. The method is successfully applied to remove the ambiguity in the transverse component of the vector magnetogram solely using observations (from HRT and from the Helioseismic and Magnetic Imager), for the first time. The SDM is proven to provide observation-only disambiguated vector magnetograms that are spatially homogeneous and consistent. A discussion about the sources of error that may limit the accuracy of the method, and of the strategies to remove them in future applications, is also presented., Comment: 32 pages, 12 figures, accepted in A&A on 09/07/2023
Published: 2023
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6. Wavefront error of PHI/HRT on Solar Orbiter at various heliocentric distances

Author: Kahil, F., Gandorfer, A., Hirzberger, J., Calchetti, D., Sinjan, J., Valori, G., Solanki, S. K., Van Noort, M., Albert, K., Jorge, N. Albelo, Alvarez-Herrero, A., Appourchaux, T., Rubio, L. R. Bellot, guez, J. Blanco Rodrí, Feller, A., Fiethe, B., Germerott, D., Gizon, L., Guerrero, L., Gutierrez-Marques, P., Kolleck, M., Korpi-Lagg, A., Michalik, H., Vacas, A. Moreno, arez, D. Orozco Su\', erez-Grande, I. P\', Kilders, E. Sanchis, Schou, J., uhle, U. Sch\", Staub, J., Strecker, H., iniesta, J. C. del Toro, Volkmer, R., and Woch, J.
Subjects: Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: We use wavefront sensing to characterise the image quality of the the High Resolution Telescope (HRT) of the Polarimetric and Helioseismic Imager (SO/PHI) data products during the second remote sensing window of the Solar Orbiter (SO) nominal mission phase. Our ultimate aims are to reconstruct the HRT data by deconvolving with the HRT point spread function (PSF) and to correct for the effects of optical aberrations on the data. We use a pair of focused--defocused images to compute the wavefront error and derive the PSF of HRT by means of a phase diversity (PD) analysis. The wavefront error of HRT depends on the orbital distance of SO to the Sun. At distances $>0.5$\,au, the wavefront error is small, and stems dominantly from the inherent optical properties of HRT. At distances $<0.5$\,au, the thermo-optical effect of the Heat Rejection Entrance Window (HREW) becomes noticeable. We develop an interpolation scheme for the wavefront error that depends on the thermal variation of the HREW with the distance of SO to the Sun. We also introduce a new level of image reconstruction, termed `aberration correction', which is designed to reduce the noise caused by image deconvolution while removing the aberrations caused by the HREW. The computed PSF via phase diversity significantly reduces the degradation caused by the HREW in the near-perihelion HRT data. In addition, the aberration correction increases the noise by a factor of only $1.45$ compared to the factor of $3$ increase that results from the usual PD reconstructions.
Published: 2023
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7. Direct assessment of SDO/HMI helioseismology of active regions on the Sun's far side using SO/PHI magnetograms

Author: Yang, D., Gizon, L., Barucq, H., Hirzberger, J., Suárez, D. Orozco, Albert, K., Jorge, N. Albelo, Appourchaux, T., Alvarez-Herrero, A., Rodríguez, J. Blanco, Gandorfer, A., Germerott, D., Guerrero, L., Gutierrez-Marques, P., Kahil, F., Kolleck, M., Solanki, S. K., Iniesta, J. C. del Toro, Volkmer, R., Woch, J., Pérez-Grande, I., Kilders, E. Sanchis, Jiménez, M. Balaguer, Rubio, L. R. Bellot, Calchetti, D., Carmona, M., Deutsch, W., Feller, A., Fernandez-Rico, G., Fernández-Medina, A., Parejo, P. García, Blesa, J. L. Gasent, Grauf, B., Heerlein, K., Korpi-Lagg, A., Lange, T., Jiménez, A. López, Maue, T., Meller, R., Vacas, A. Moreno, Müller, R., Nakai, E., Schmidt, W., Schou, J., Schühle, U., Sinjan, J., Staub, J., Strecker, H., Torralbo, I., and Valori, G.
Subjects: Astrophysics - Solar and Stellar Astrophysics
Abstract: Earth-side observations of solar p modes can be used to image and monitor magnetic activity on the Sun's far side. Here we use magnetograms of the far side obtained by the Polarimetric and Helioseismic Imager (PHI) onboard Solar Orbiter (SO) to directly assess -- for the first time -- the validity of far-side helioseismic holography. We wish to co-locate the positions of active regions in helioseismic images and magnetograms, and to calibrate the helioseismic measurements in terms of magnetic field strength. We identify three magnetograms on 18 November 2020, 3 October 2021, and 3 February 2022 displaying a total of six active regions on the far side. The first two dates are from SO's cruise phase, the third from the beginning of the nominal operation phase. We compute contemporaneous seismic phase maps for these three dates using helioseismic holography applied to time series of Dopplergrams from the Helioseismic and Magnetic Imager (HMI) on the Solar Dynamics Observatory (SDO). Among the six active regions seen in SO/PHI magnetograms, five active regions are identified on the seismic maps at almost the same positions as on the magnetograms. One region is too weak to be detected above the seismic noise. To calibrate the seismic maps, we fit a linear relationship between the seismic phase shifts and the unsigned line-of-sight magnetic field averaged over the active region areas extracted from the SO/PHI magnetograms. SO/PHI provides the strongest evidence so far that helioseismic imaging provides reliable information about active regions on the far side, including their positions, areas, and mean unsigned magnetic field., Comment: 10 pages, 9 figures
Published: 2023
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8. Spectropolarimetric investigation of magnetohydrodynamic wave modes in the photosphere: First results from PHI on board Solar Orbiter

Author: Calchetti, D., Stangalini, M., Jafarzadeh, S., Valori, G., Albert, K., Jorge, N. Albelo, Alvarez-Herrero, A., Appourchaux, T., Jiménez, M. Balaguer, Rubio, L. R. Bellot, Rodríguez, J. Blanco, Feller, A., Gandorfer, A., Germerott, D., Gizon, L., Guerrero, L., Gutierrez-Marques, P., Hirzberger, J., Kahil, F., Kolleck, M., Korpi-Lagg, A., Vacas, A. Moreno, Suárez, D. Orozco, Pérez-Grande, I., Kilders, E. Sanchis, Schou, J., Schühle, U., Sinjan, J., Solanki, S. K., Staub, J., Strecker, H., Iniesta, J. C. del Toro, Volkmer, R., and Woch, J.
Subjects: Astrophysics - Solar and Stellar Astrophysics
Abstract: In November 2021, Solar Orbiter started its nominal mission phase. The remote-sensing instruments on board the spacecraft acquired scientific data during three observing windows surrounding the perihelion of the first orbit of this phase. The aim of the analysis is the detection of magnetohydrodynamic (MHD) wave modes in an active region by exploiting the capabilities of spectropolarimetric measurements. The High Resolution Telescope (HRT) of the Polarimetric and Helioseismic Imager (SO/PHI) on board the Solar Orbiter acquired a high-cadence data set of an active region. This is studied in the paper. B-$\omega$ and phase-difference analyses are applied on line-of-sight velocity and circular polarization maps and other averaged quantities. We find that several MHD modes at different frequencies are excited in all analysed structures. The leading sunspot shows a linear dependence of the phase lag on the angle between the magnetic field and the line of sight of the observer in its penumbra. The magnetic pore exhibits global resonances at several frequencies, which are also excited by different wave modes. The SO/PHI measurements clearly confirm the presence of magnetic and velocity oscillations that are compatible with one or more MHD wave modes in pores and a sunspot. Improvements in modelling are still necessary to interpret the relation between the fluctuations of different diagnostics.
Published: 2023
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9. The ratio of horizontal to vertical displacement in solar oscillations estimated from combined SO/PHI and SDO/HMI observations

Author: Schou, J., Hirzberger, J., Suárez, D. Orozco, Albert, K., Jorge, N. Albelo, Appourchaux, T., Alvarez-Herrero, A., Rodríguez, J. Blanco, Gandorfer, A., Germerott, D., Guerrero, L., Gutierrez-Marques, P., Kahil, F., Kolleck, M., Solanki, S. K., Iniesta, J. C. del Toro, Volkmer, R., Woch, J., Fiethe, B., Pérez-Grande, I., Kilders, E. Sanchis, Jiménez, M. Balaguer, Rubio, L. R. Bellot, Calchetti, D., Carmona, M., Deutsch, W., Feller, A., Fernandez-Rico, G., Fernández-Medina, A., Parejo, P. García, Blesa, J. L. Gasent, Gizon, L., Grauf, B., Heerlein, K., Korpi-Lagg, A., Jiménez, A. López, Maue, T., Meller, R., Vacas, A. Moreno, Müller, R., Nakai, E., Schmidt, W., Sinjan, J., Staub, J., Strecker, H., Torralbo, I., and Valori, G.
Subjects: Astrophysics - Solar and Stellar Astrophysics
Abstract: In order to make accurate inferences about the solar interior using helioseismology, it is essential to understand all the relevant physical effects on the observations. One effect to understand is the (complex-valued) ratio of the horizontal to vertical displacement of the p- and f-modes at the height at which they are observed. Unfortunately, it is impossible to measure this ratio directly from a single vantage point, and it has been difficult to disentangle observationally from other effects. In this paper we attempt to measure the ratio directly using 7.5 hours of simultaneous observations from the Polarimetric and Helioseismic Imager on board Solar Orbiter and the Helioseismic and Magnetic Imager on board the Solar Dynamics Observatory. While image geometry problems make it difficult to determine the exact ratio, it appears to agree well with that expected from adiabatic oscillations in a standard solar model. On the other hand it does not agree with a commonly used approximation, indicating that this approximation should not be used in helioseismic analyses. In addition, the ratio appears to be real-valued., Comment: Accepted for publication in Astronomy & Astrophysics. 8 pages, 8 figures
Published: 2023
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10. Magnetic fields inferred by Solar Orbiter: A comparison between SO/PHI-HRT and SDO/HMI

Author: Sinjan, J., Calchetti, D., Hirzberger, J., Kahil, F., Valori, G., Solanki, S. K., Albert, K., Jorge, N. Albelo, Alvarez-Herrero, A., Appourchaux, T., Rubio, L. R. Bellot, Rodríguez, J. Blanco, Feller, A., Gandorfer, A., Germerott, D., Gizon, L., Cama, J. M. Gómez, Guerrero, L., Gutierrez-Marques, P., Kolleck, M., Korpi-Lagg, A., Michalik, H., Vacas, A. Moreno, Suárez, D. Orozco, Pérez-Grande, I., Kilders, E. Sanchis, Jiménez, M. Balaguer, Schou, J., Schühle, U., Staub, J., Strecker, H., Iniesta, J. C. del Toro, Volkmer, R., and Woch, J.
Subjects: Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Earth and Planetary Astrophysics, Physics - Space Physics
Abstract: The High Resolution Telescope (HRT) of the Polarimetric and Helioseismic Imager on board the Solar Orbiter spacecraft (SO/PHI) and the Helioseismic and Magnetic Imager (HMI) on board the Solar Dynamics Observatory (SDO) both infer the photospheric magnetic field from polarised light images. SO/PHI is the first magnetograph to move out of the Sun--Earth line and will provide unprecedented access to the Sun's poles. This provides excellent opportunities for new research wherein the magnetic field maps from both instruments are used simultaneously. We aim to compare the magnetic field maps from these two instruments and discuss any possible differences between them. We used data from both instruments obtained during Solar Orbiter's inferior conjunction on 7 March 2022. The HRT data were additionally treated for geometric distortion and degraded to the same resolution as HMI. The HMI data were re-projected to correct for the $3^{\circ}$ separation between the two observatories. SO/PHI-HRT and HMI produce remarkably similar line-of-sight magnetograms, with a slope coefficient of $0.97$, an offset below $1$ G, and a Pearson correlation coefficient of $0.97$. However, SO/PHI-HRT infers weaker line-of-sight fields for the strongest fields. As for the vector magnetic field, SO/PHI-HRT was compared to both the $720$-second and $90$-second HMI vector magnetic field: SO/PHI-HRT has a closer alignment with the $90$-second HMI vector. In the weak signal regime ($< 600$ G), SO/PHI-HRT measures stronger and more horizontal fields than HMI, very likely due to the greater noise in the SO/PHI-HRT data. In the strong field regime ($\gtrsim 600$ G), HRT infers lower field strengths but with similar inclinations (a slope of $0.92$) and azimuths (a slope of $1.02$). The slope values are from the comparison with the HMI $90$-second vector., Comment: 10 pages, 5 figures, accepted for publication in A&A; manuscript is a part of Astronomy & Astrophysics special issue: Solar Orbiter First Results (Nominal Mission Phase)
Published: 2023
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11. The on-ground data reduction and calibration pipeline for SO/PHI-HRT

Author: Sinjan, J., Calchetti, D., Hirzberger, J., Suárez, D. Orozco, Albert, K., Jorge, N. Albelo, Appourchaux, T., Alvarez-Herrero, A., Rodríguez, J. Blanco, Gandorfer, A., Germerott, D., Guerrero, L., Marquez, P. Gutierrez, Kahil, F., Kolleck, M., Solanki, S. K., Iniesta, J. C. del Toro, Volkmer, R., Woch, J., Fiethe, B., Cama, J. M. Gómez, Pérez-Grande, I., Kilders, E. Sanchis, Jiménez, M. Balaguer, Rubio, L. R. Bellot, Carmona, M., Deutsch, W., Fernandez-Rico, G., Fernández-Medina, A., Parejo, P. García, Blesa, J. L. Gasent, Gizon, L., Grauf, B., Heerlein, K., Korpi-Lagg, A., Lange, T., Jiménez, A. López, Maue, T., Meller, R., Michalik, H., Vacas, A. Moreno, Müller, R., Nakai, E., Schmidt, W., Schou, J., Schühle, U., Staub, J., Strecker, H., Torralbo, I., and Valori, G.
Subjects: Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: The ESA/NASA Solar Orbiter space mission has been successfully launched in February 2020. Onboard is the Polarimetric and Helioseismic Imager (SO/PHI), which has two telescopes, a High Resolution Telescope (HRT) and the Full Disc Telescope (FDT). The instrument is designed to infer the photospheric magnetic field and line-of-sight velocity through differential imaging of the polarised light emitted by the Sun. It calculates the full Stokes vector at 6 wavelength positions at the Fe I 617.3 nm absorption line. Due to telemetry constraints, the instrument nominally processes these Stokes profiles onboard, however when telemetry is available, the raw images are downlinked and reduced on ground. Here the architecture of the on-ground pipeline for HRT is presented, which also offers additional corrections not currently available on board the instrument. The pipeline can reduce raw images to the full Stokes vector with a polarimetric sensitivity of $10^{-3}\cdot I_{c}$ or better.
Published: 2022
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12. The magnetic drivers of campfires seen by the Polarimetric and Helioseismic Imager (PHI) on Solar Orbiter

Author: Kahil, F., Hirzberger, J., Solanki, S. K., Chitta, L. P., Peter, H., Auchère, F., Sinjan, J., Suárez, D. Orozco, Albert, K., Jorge, N. Albelo, Appourchaux, T., Alvarez-Herrero, A., Rodríguez, J. Blanco, Gandorfer, A., Germerott, D., Guerrero, L., Márquez, P. Gutiérrez, Kolleck, M., Iniesta, J. C. del Toro, Volkmer, R., Woch, J., Fiethe, B., Cama, J. M. Gómez, Pérez-Grande, I., Kilders, E. Sanchis, Jiménez, M. Balaguer, Rubio, L. R. Bellot, Calchetti, D., Carmona, M., Deutsch, W., Fernández-Rico, G., Fernández-Medina, A., Parejo, P. García, Gasent-Blesa, J. L., Gizon, L., Grauf, B., Heerlein, K., Lagg, A., Lange, T., Jiménez, A. López, Maue, T., Meller, R., Michalik, H., Vacas, A. Moreno, uller, R. M\", Nakai, E., Schmidt, W., Schou, J., Schühle, U., Staub, J., Strecker, H., Torralbo, I., Valori, G., Cuadrado, R. Aznar, Teriaca, L., Berghmans, D., Verbeeck, C., Kraaikamp, E., and Gissot, S.
Subjects: Astrophysics - Solar and Stellar Astrophysics, Physics - Space Physics
Abstract: The Extreme Ultraviolet Imager (EUI) on board the Solar Orbiter (SO) spacecraft observed small extreme ultraviolet (EUV) bursts, termed campfires, that have been proposed to be brightenings near the apexes of low-lying loops in the quiet-Sun atmosphere. The underlying magnetic processes driving these campfires are not understood. During the cruise phase of SO and at a distance of 0.523\,AU from the Sun, the Polarimetric and Helioseismic Imager on Solar Orbiter (SO/PHI) observed a quiet-Sun region jointly with SO/EUI, offering the possibility to investigate the surface magnetic field dynamics underlying campfires at a spatial resolution of about 380~km. In 71\% of the 38 isolated events, campfires are confined between bipolar magnetic features, which seem to exhibit signatures of magnetic flux cancellation. The flux cancellation occurs either between the two main footpoints, or between one of the footpoints of the loop housing the campfire and a nearby opposite polarity patch. In one particularly clear-cut case, we detected the emergence of a small-scale magnetic loop in the internetwork followed soon afterwards by a campfire brightening adjacent to the location of the linear polarisation signal in the photosphere, that is to say near where the apex of the emerging loop lays. The rest of the events were observed over small scattered magnetic features, which could not be identified as magnetic footpoints of the campfire hosting loops. The majority of campfires could be driven by magnetic reconnection triggered at the footpoints, similar to the physical processes occurring in the burst-like EUV events discussed in the literature. About a quarter of all analysed campfires, however, are not associated to such magnetic activity in the photosphere, which implies that other heating mechanisms are energising these small-scale EUV brightenings.
Published: 2022
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13. JEM-EUSO Collaboration contributions to the 37th International Cosmic Ray Conference

Author: Abdellaoui, G., Abe, S., Adams Jr., J. H., Allard, D., Alonso, G., Anchordoqui, L., Anzalone, A., Arnone, E., Asano, K., Attallah, R., Attoui, H., Pernas, M. Ave, Bagheri, M., Baláz, J., Bakiri, M., Barghini, D., Bartocci, S., Battisti, M., Bayer, J., Beldjilali, B., Belenguer, T., Belkhalfa, N., Bellotti, R., Belov, A. A., Benmessai, K., Bertaina, M., Bertone, P. F., Biermann, P. L., Bisconti, F., Blaksley, C., Blanc, N., Blin-Bondil, S., Bobik, P., Bogomilov, M., Bolmgren, K., Bozzo, E., Briz, S., Bruno, A., Caballero, K. S., Cafagna, F., Cambié, G., Campana, D., Capdevielle, J-N., Capel, F., Caramete, A., Caramete, L., Carlson, P., Caruso, R., Casolino, M., Cassardo, C., Castellina, A., Catalano, O., Cellino, A., Černý, K., Chikawa, M., Chiritoi, G., Christl, M. J., Colalillo, R., Conti, L., Cotto, G., Crawford, H. J., Cremonini, R., Creusot, A., Gónzalez, A. de Castro, de la Taille, C., del Peral, L., Damian, A. Diaz, Diesing, R., Dinaucourt, P., Djakonow, A., Djemil, T., Ebersoldt, A., Ebisuzaki, T., Eser, J., Fenu, F., Fernández-González, S., Ferrarese, S., Filippatos, G., Fornaro, W. I. Finch C., Fouka, M., Franceschi, A., Franchini, S., Fuglesang, C., Fujii, T., Fukushima, M., Galeotti, P., García-Ortega, E., Gardiol, D., Garipov, G. K., Gascón, E., Gazda, E., Genci, J., Golzio, A., Alvarado, C. González, Gorodetzky, P., Green, A., Guarino, F., Guépin, C., Guzmán, A., Hachisu, Y., Haungs, A., Carretero, J. Hernández, Hulett, L., Ikeda, D., Inoue, N., Inoue, S., Isgrò, F., Itow, Y., Jammer, T., Jeong, S., Joven, E., Judd, E. G., Jochum, J., Kajino, F., Kajino, T., Kalli, S., Kaneko, I., Karadzhov, Y., Kasztelan, M., Katahira, K., Kawai, K., Kawasaki, Y., Kedadra, A., Khales, H., Khrenov, B. A., Kim, Jeong-Sook, Kim, Soon-Wook, Kleifges, M., Klimov, P. A., Kolev, D., Kreykenbohm, I., Krizmanic, J. F., Królik, K., Kungel, V., Kurihara, Y., Kusenko, A., Kuznetsov, E., Lahmar, H., Lakhdari, F., Licandro, J., Campano, L. López, Martínez, F. López, Mackovjak, S., Mahdi, M., Mandát, D., Manfrin, M., Marcelli, L., Marcos, J. L., Marszał, W., Martín, Y., Martinez, O., Mase, K., Matev, R., Matthews, J. N., Mebarki, N., Medina-Tanco, G., Menshikov, A., Merino, A., Mese, M., Meseguer, J., Meyer, S. S., Mimouni, J., Miyamoto, H., Mizumoto, Y., Monaco, A., Ríos, J. A. Morales de los, Mastafa, M., Nagataki, S., Naitamor, S., Napolitano, T., Neronov, J. M. Nachtman A., Nomoto, K., Nonaka, T., Ogawa, T., Ogio, S., Ohmori, H., Olinto, A. V., Osteria, Y. Onel G., Otte, A. N., Pagliaro, A., Painter, W., Panasyuk, M. I., Panico, B., Parizot, E., Park, I. H., Pastircak, B., Paul, T., Pech, M., Pérez-Grande, I., Perfetto, F., Peter, T., Picozza, P., Pindado, S., Piotrowski, L. W., Piraino, S., Plebaniak, Z., Pollini, A., Popescu, E. M., Prevete, R., Prévôt, G., Prieto, H., Przybylak, M., Puehlhofer, G., Putis, M., Reardon, P., Reno, M. H., Reyes, M., Ricci, M., Frías, M. D. Rodríguez, Matamala, O. F. Romero, Ronga, F., Sabau, M. D., Saccá, G., Cano, G. Sáez, Sagawa, H., Sahnoune, Z., Saito, A., Sakaki, N., Salazar, H., Balanzar, J. C. Sanchez, Sánchez, J. L., Santangelo, A., Sanz-Andrés, A., Palomino, M. Sanz, Saprykin, O. A., Sarazin, F., Sato, M., Scagliola, A., Schanz, T., Schieler, H., Schovánek, P., Scotti, V., Serra, M., Sharakin, S. A., Shimizu, H. M., Shinozaki, K., Soriano, J. F., Sotgiu, A., Stan, I., Strharský, I., Sugiyama, N., Supanitsky, D., Suzuki, M., Szabelski, J., Tajima, N., Tajima, T., Takahashi, Y., Takeda, M., Takizawa, Y., Talai, M. C., Tameda, Y., Tenzer, C., Thomas, S. B., Tibolla, O., Tkachev, L. G., Tomida, T., Tone, N., Toscano, S., Traïche, M., Tsunesada, Y., Tsuno, K., Turriziani, S., Uchihori, Y., Vaduvescu, O., Valdés-Galicia, J. F., Vallania, P., Valore, L., Vankova-Kirilova, G., Venters, T. M., Vigorito, C., Villaseñor, L., Vlcek, B., von Ballmoos, P., Vrabel, M., Wada, S., Watanabe, J., Watts Jr., J., Muñoz, R. Weigand, Weindl, A., Wiencke, L., Wille, M., Wilms, J., Yamamoto, D. Winn T., Yang, J., Yano, H., Yashin, I. V., Yonetoku, D., Yoshida, S., Young, R., Zgura, I. S., Zotov, M. Yu., and Marchi, A. Zuccaro
Subjects: Astrophysics - High Energy Astrophysical Phenomena
Abstract: Compilation of papers presented by the JEM-EUSO Collaboration at the 37th International Cosmic Ray Conference (ICRC), held on July 12-23, 2021 (online) in Berlin, Germany., Comment: html page with links to the JEM-EUSO Collaboration papers presented at ICRC-2021, Berlin, Germany
Published: 2022

14. The mediating role of reflective functioning in the association between childhood trauma and suicide attempt

Author: Palao-Tarrero, A., Vicente, L., Velasco, M., Orgaz, B., García, D., Vieta, E., Vázquez, M., Bracco, L., Gómez-Vallejo, S., Díaz, C., Palao, D.J., Comendador, L., Punti, J., Muñoz, M.T., García- Ramos, A., Ayad-Ahmed, W., Diaz-Carracedo, P., Ayuso-Mateos, J.L., Jimenez-Treviño, L., Bobes-Bascarán, M.T., Seijo-Zazo, E., Fernandez-Fernandez, J., Garcia-Fernandez, A., Canal-Rivero, M., Rider, J., Reguera, P., Puertas, M., García-Ligero, E., Tur, N., Navas, M., Saiz-Gonzalez, D., Carrasco, J.L., Andreo-Jover, J., Curto Ramos, J., Bobes, J., Bravo-Ortiz, M., Cebria, A.I., Crespo-Facorro, B., De la Torre-Luque, A., Díaz-Marsa, M., Fernández-Rodrigues, V., Garrido-Torres, N., Grande, I., López Peña, M.P., Pemau, A., Roberto, N., Ruiz-Veguilla, M., Saiz, P., Rodríguez-Vega, B., and Pérez-Sola, V.
Published: 2024
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15. EUSO-SPB1 mission and science

Author: Abdellaoui, G., Abe, S., Adams, J.H., Jr., Allard, D., Alonso, G., Anchordoqui, L., Anzalone, A., Arnone, E., Asano, K., Attallah, R., Attoui, H., Pernas, M. Ave, Bachmann, R., Bacholle, S., Bagheri, M., Bakiri, M., Baláz, J., Barghini, D., Bartocci, S., Battisti, M., Bayer, J., Beldjilali, B., Belenguer, T., Belkhalfa, N., Bellotti, R., Belov, A.A., Benmessai, K., Bertaina, M., Bertone, P.F., Biermann, P.L., Bisconti, F., Blaksley, C., Blanc, N., Blin-Bondil, S., Bobik, P., Bogomilov, M., Bolmgren, K., Bozzo, E., Briz, S., Bruno, A., Caballero, K.S., Cafagna, F., Cambié, G., Campana, D., Capdevielle, J.N., Capel, F., Caramete, A., Caramete, L., Caruso, R., Casolino, M., Cassardo, C., Castellina, A., Catalano, O., Cellino, A., Černý, K., Chikawa, M., Chiritoi, G., Christl, M.J., Colalillo, R., Conti, L., Cotto, G., Crawford, H.J., Cremonini, R., Creusot, A., Cummings, A., de Castro Gónzalez, A., de la Taille, C., del Peral, L., Desiato, J., Damian, A. Diaz, Diesing, R., Dinaucourt, P., Djakonow, A., Djemil, T., Ebersoldt, A., Ebisuzaki, T., Eser, J., Fenu, F., Fernández-González, S., Ferrarese, S., Filippatos, G., Finch, W., Fornaro, C., Fouka, M., Franceschi, A., Franchini, S., Fuglesang, C., Fujii, T., Fukushima, M., Galeotti, P., García-Ortega, E., Gardiol, D., Garipov, G.K., Gascón, E., Gazda, E., Genci, J., Golzio, A., Gorodetzky, P., Gregg, R., Green, A., Guarino, F., Guépin, C., Guzmán, A., Hachisu, Y., Haungs, A., Heigbes, T., Carretero, J. Hernández, Hulett, L., Ikeda, D., Inoue, N., Inoue, S., Isgrò, F., Itow, Y., Jammer, T., Jeong, S., Jochum, J., Joven, E., Judd, E.G., Jung, A., Kajino, F., Kajino, T., Kalli, S., Kaneko, I., Kasztelan, M., Katahira, K., Kawai, K., Kawasaki, Y., Kedadra, A., Khales, H., Khrenov, B.A., Kim, Jeong-Sook, Kim, Soon-Wook, Kleifges, M., Klimov, P.A., Kreykenbohm, I., Krizmanic, J.F., Królik, K., Kungel, V., Kurihara, Y., Kusenko, A., Kuznetsov, E., Lahmar, H., Lakhdari, F., Licandro, J., Campano, L. López, Martínez, F. López, Mackovjak, S., Mahdi, M., Mandát, D., Manfrin, M., Marcelli, L., Marcos, J.L., Marszał, W., Martín, Y., Martinez, O., Mase, K., Mastafa, M., Matthews, J.N., Mebarki, N., Medina-Tanco, G., Menshikov, A., Merino, A., Mese, M., Meseguer, J., Meyer, S.S., Mimouni, J., Miyamoto, H., Mizumoto, Y., Monaco, A., de los Ríos, J.A. Morales, Nachtman, J.M., Nagataki, S., Naitamor, S., Napolitano, T., Neronov, A., Nomoto, K., Nonaka, T., Ogawa, T., Ogio, S., Ohmori, H., Olinto, A.V., Onel, Y., Osteria, G., Otte, A.N., Pagliaro, A., Painter, W., Panasyuk, M.I., Panico, B., Parizot, E., Park, I.H., Pastircak, B., Paul, T., Pech, M., Pérez-Grande, I., Perfetto, F., Peter, T., Picozza, P., Pindado, S., Piotrowski, L.W., Piraino, S., Plebaniak, Z., Pollini, A., Popescu, E.M., Prevete, R., Prévôt, G., Prieto, H., Przybylak, M., Puehlhofer, G., Putis, M., Reardon, P., Reno, M.H., Reyes, M., Ricci, M., Frías, M.D. Rodríguez, Matamala, O.F. Romero, Ronga, F., Sabau, M.D., Saccá, G., Sagawa, H., Sahnoune, Z., Saito, A., Sakaki, N., Salazar, H., Sánchez, J.L., Balanzar, J.C. Sanchez, Santangelo, A., Sanz-Andrés, A., Saprykin, O.A., Sarazin, F., Sato, M., Scagliola, A., Schanz, T., Schieler, H., Schovánek, P., Scotti, V., Serra, M., Sharakin, S.A., Shimizu, H.M., Shinozaki, K., Soriano, J.F., Sotgiu, A., Stan, I., Strharský, I., Sugiyama, N., Supanitsky, D., Suzuki, M., Szabelski, J., Tajima, N., Tajima, T., Takahashi, Y., Takeda, M., Takizawa, Y., Talai, M.C., Tameda, Y., Tenzer, C., Thomas, S.B., Tibolla, O., Tkachev, L.G., Tomida, T., Tone, N., Toscano, S., Traïche, M., Tsunesada, Y., Tsuno, K., Turriziani, S., Uchihori, Y., Valdés-Galicia, J.F., Vallania, P., Valore, L., Vankova-Kirilova, G., Venters, T.M., Vigorito, C., Villaseñor, L., Vlcek, B., von Ballmoos, P., Vrabel, M., Wada, S., Watanabe, J., Watts, J., Jr., Muñoz, R. Weigand, Weindl, A., Wiencke, L., Wille, M., Wilms, J., Yamamoto, T., Yang, J., Yano, H., Yashin, I.V., Yonetoku, D., Yoshida, S., Young, R., Zgura, I.S., Zotov, M.Yu., and Marchi, A. Zuccaro
Published: 2024
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16. The diverse meteorology of Jezero crater over the first 250 sols of Perseverance on Mars

Author: Rodriguez-Manfredi, J. A., de la Torre Juarez, M., Sanchez-Lavega, A., Hueso, R., Martinez, G., Lemmon, M. T., Newman, C. E., Munguira, A., Hieta, M., Tamppari, L. K., Polkko, J., Toledo, D., Sebastian, E., Smith, M. D., Jaakonaho, I., Genzer, M., De Vicente-Retortillo, A., Viudez-Moreiras, D., Ramos, M., Saiz-Lopez, A., Lepinette, A., Wolff, M., Sullivan, R. J., Gomez-Elvira, J., Apestigue, V., Conrad, P. G., Del Rio-Gaztelurrutia, T., Murdoch, N., Arruego, I., Banfield, D., Boland, J., Brown, A. J., Ceballos, J., Dominguez-Pumar, M., Espejo, S., Fairén, A. G., Ferrandiz, R., Fischer, E., Garcia-Villadangos, M., Gimenez, S., Gomez-Gomez, F., Guzewich, S. D., Harri, A.-M., Jimenez, J. J., Jimenez, V., Makinen, T., Marin, M., Martin, C., Martin-Soler, J., Molina, A., Mora-Sotomayor, L., Navarro, S., Peinado, V., Perez-Grande, I., Pla-Garcia, J., Postigo, M., Prieto-Ballesteros, O., Rafkin, S. C. R., Richardson, M. I., Romeral, J., Romero, C., Savijärvi, H., Schofield, J. T., Torres, J., Urqui, R., and Zurita, S.
Published: 2023
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17. Contributions to the 36th International Cosmic Ray Conference (ICRC 2019) of the JEM-EUSO Collaboration

Author: Abdellaoui, G., Abe, S., Adams Jr., J. H., Ahriche, A., Allard, D., Allen, L., Alonso, G., Anchordoqui, L., Anzalone, A., Arai, Y., Asano, K., Attallah, R., Attoui, H., Pernas, M. Ave, Bacholle, S., Bakiri, M., Baragatti, P., Barrillon, P., Bartocci, S., Bayer, J., Beldjilali, B., Belenguer, T., Belkhalfa, N., Bellotti, R., Belov, A., Belov, K., Benmessai, K., Bertaina, M., Biermann, P. L., Biktemerova, S., Bisconti, F., Blaksley, C., Blanc, N., Błęcki, J., Blin-Bondil, S., Bobik, P., Bogomilov, M., Bozzo, E., Pacheco, S. Briz, Bruno, A., Caballero, K. S., Cafagna, F., Campana, D., Capdevielle, J-N., Capel, F., Caramete, A., Caramete, L., Carlson, P., Caruso, R., Casolino, M., Cassardo, C., Castellina, A., Catalano, O., Cellino, A., Chikawa, M., Chiritoi, G., Christl, M. J., Connaughton, V., Conti, L., Cotto, G., Crawford, H. J., Cremonini, R., Creusot, A., Csorna, S., Cummings, A., Dagoret-Campagne, S., Gónzalez, A. de Castro, De Donato, C., de la Taille, C., De Santis, C., del Peral, L., Di Martino, M., Damian, A. Diaz, Djemil, T., Dutan, I., Ebersoldt, A., Ebisuzaki, T., Engel, R., Eser, J., Fenu, F., Fernández-González, S., Ferrarese, S., Flamini, M., Fornaro, C., Fouka, M., Franceschi, A., Franchini, S., Fuglesang, C., Fujii, T., Fujimoto, J., Fukushima, M., Galeotti, P., García-Ortega, E., Garipov, G., Gascón, E., Genci, J., Giraudo, G., Alvarado, C. González, Gorodetzky, P., Greg, R., Guarino, F., Guzmán, A., Hachisu, Y., Haiduc, M., Harlov, B., Haungs, A., Carretero, J. Hernández, Cruz, W. Hidber, Ikeda, D., Inoue, N., Inoue, S., Isgrò, F., Itow, Y., Jammer, T., Jeong, S., Joven, E., Judd, E. G., Jung, A., Jochum, J., Kajino, F., Kajino, T., Kalli, S., Kaneko, I., Karadzhov, Y., Karczmarczyk, J., Katahira, K., Kawai, K., Kawasaki, Y., Kedadra, A., Khales, H., Khrenov, B. A., Kim, Jeong-Sook, Kim, Soon-Wook, Kleifges, M., Klimov, P. A., Kolev, D., Krantz, H., Kreykenbohm, I., Krizmanic, J. F., Kudela, K., Kurihara, Y., Kusenko, A., Kuznetsov, E., La Barbera, A., Lahmar, H., Lakhdari, F., Larsson, O., Lee, J., Licandro, J., Campano, L. López, Martínez, F. López, Maccarone, M. C., Mackovjak, S., Mahdi, M., Maravilla, D., Marcelli, L., Marcos, J. L., Marini, A., Marszał, W., Martens, K., Martín, Y., Martinez, O., Martucci, M., Masciantonio, G., Mase, K., Matev, R., Matthews, J. N., Mebarki, N., Medina-Tanco, G., Menshikov, A., Merino, A., Meseguer, J., Meyer, S. S., Mimouni, J., Miyamoto, H., Mizumoto, Y., Monaco, A., Ríos, J. A. Morales de los, Mustafa, M., Nagataki, S., Naitamor, S., Napolitano, T., Nava, R., Neronov, A., Nomoto, K., Nonaka, T., Ogawa, T., Ogio, S., Ohmori, H., Olinto, A. V., Orleaánski, P., Osteria, G., Pagliaro, A., Painter, W., Panasyuk, M. I., Panico, B., Parizot, E., Park, I. H., Pastircak, B., Patzak, T., Paul, T., Pérez-Grande, I., Perfetto, F., Peter, T., Picozza, P., Pindado, S., Piotrowski, L. W., Piraino, S., Placidi, L., Plebaniak, Z., Pliego, S., Pollini, A., Polonski, Z., Popescu, E. M., Prat, P., Prévôt, G., Prieto, H., Puehlhofer, G., Putis, M., Rabanal, J., Radu, A. A., Reyes, M., Rezazadeh, M., Ricci, M., Frías, M. D. Rodríguez, Ronga, F., Roudil, G., Rusinov, I., Rybczyński, M., Sabau, M. D., Cano, G. Sáaez, Sagawa, H., Sahnoune, Z., Saito, A., Sakaki, N., Salazar, H., Balanzar, J. C. Sanchez, Sánchez, J. L., Santangelo, A., Sanz-Andrés, A., Palomino, M. Sanz, Saprykin, O., Sarazin, F., Sato, M., Schanz, T., Schieler, H., Scotti, V., Selmane, S., Semikoz, D., Serra, M., Sharakin, S., Shimizu, H. M., Shinozaki, K., Shirahama, T., Spataro, B., Stan, I., Sugiyama, T., Supanitsky, D., Suzuki, M., Szabelska, B., Szabelski, J., Tajima, N., Tajima, T., Takahashi, Y., Takami, H., Takeda, M., Takizawa, Y., Talai, M. C., Tenzer, C., Thomas, S. B., Tibolla, O., Tkachev, L., Tokuno, H., Tomida, T., Tone, N., Toscano, S., Traïche, M., Tsenov, R., Tsunesada, Y., Tsuno, K., Tubbs, J., Turriziani, S., Uchihori, Y., Vaduvescu, O., Valdés-Galicia, J. F., Vallania, P., Vankova, G., Vigorito, C., Villaseñor, L., Vlcek, B., von Ballmoos, P., Vrabel, M., Wada, S., Watanabe, J., Watts Jr., J., Weber, M., Muñoz, R. Weigand, Weindl, A., Wiencke, L., Wille, M., Wilms, J., Włodarczyk, Z., Yamamoto, T., Yang, J., Yano, H., Yashin, I. V., Yonetoku, D., Yoshida, S., Young, R., Zgura, I. S, Zotov, M. Yu., and Marchi, A. Zuccaro
Subjects: Astrophysics - High Energy Astrophysical Phenomena
Abstract: Compilation of papers presented by the JEM-EUSO Collaboration at the 36th International Cosmic Ray Conference (ICRC), held July 24 through August 1, 2019 in Madison, Wisconsin., Comment: links to the 24 papers published in arXiv
Published: 2019

18. The Polarimetric and Helioseismic Imager on Solar Orbiter

Author: Solanki, S. K., Iniesta, J. C. del Toro, Woch, J., Gandorfer, A., Hirzberger, J., Alvarez-Herrero, A., Appourchaux, T., Pillet, V. Martínez, Pérez-Grande, I., Kilders, E. Sanchis, Schmidt, W., Cama, J. M. Gómez, Michalik, H., Deutsch, W., Fernandez-Rico, G., Grauf, B., Gizon, L., Heerlein, K., Kolleck, M., Lagg, A., Meller, R., Müller, R., Schühle, U., Staub, J., Albert, K., Copano, M. Alvarez, Beckmann, U., Bischoff, J., Busse, D., Enge, R., Frahm, S., Germerott, D., Guerrero, L., Löptien, B., Meierdierks, T., Oberdorfer, D., Papagiannaki, I., Ramanath, S., Schou, J., Werner, S., Yang, D., Zerr, A., Bergmann, M., Bochmann, J., Heinrichs, J., Meyer, S., Monecke, M., Müller, M. -F., Sperling, M., a, D. Álvarez Garcí, Aparicio, B., Jiménez, M. Balaguer, Rubio, L. R. Bellot, Carracosa, J. P. Cobos, Girela, F., Expósito, D. Hernández, Herranz, M., Labrousse, P., Jiménez, A. López, Suárez, D. Orozco, Ramos, J. L., Barandiarán, J., Bastide, L., Campuzano, C., Cebollero, M., Dávila, B., Fernández-Medina, A., Parejo, P. García, Garranzo-García, D., Laguna, H., Martín, J. A., Navarro, R., Peral, A. Núñez, Royo, M., Sánchez, A., Silva-López, M., Vera, I., Villanueva, J., Fourmond, J. -J., de Galarreta, C. Ruiz, Bouzit, M., Hervier, V., Clec'h, J. C. Le, Szwec, N., Chaigneau, M., Buttice, V., Dominguez-Tagle, C., Philippon, A., Boumier, P., Cocguen, R. Le, Baranjuk, G., Bell, A., Berkefeld, Th., Baumgartner, J., Heidecke, F., Maue, T., Nakai, E., Scheiffelen, T., Sigwarth, M., Soltau, D., Volkmer, R., Rodríguez, J. Blanco, Domingo, V., Sabater, A. Ferreres, Blesa, J. L. Gasent, Martínez, P. Rodríguez, Caudel, D. Osorno, Bosch, J., Casas, A., Carmona, M., Herms, A., Roma, D., Alonso, G., omez-Sanjuan, A. G\', Piqueras, J., Torralbo, I., Fiethe, B., Guan, Y., Lange, T., Michel, H., Bonet, J. A., Fahmy, S., Müller, D., and Zouganelis, I.
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Astrophysics of Galaxies
Abstract: This paper describes the Polarimetric and Helioseismic Imager on the Solar Orbiter mission (SO/PHI), the first magnetograph and helioseismology instrument to observe the Sun from outside the Sun-Earth line. It is the key instrument meant to address the top-level science question: How does the solar dynamo work and drive connections between the Sun and the heliosphere? SO/PHI will also play an important role in answering the other top-level science questions of Solar Orbiter, as well as hosting the potential of a rich return in further science. SO/PHI measures the Zeeman effect and the Doppler shift in the FeI 617.3nm spectral line. To this end, the instrument carries out narrow-band imaging spectro-polarimetry using a tunable LiNbO_3 Fabry-Perot etalon, while the polarisation modulation is done with liquid crystal variable retarders (LCVRs). The line and the nearby continuum are sampled at six wavelength points and the data are recorded by a 2kx2k CMOS detector. To save valuable telemetry, the raw data are reduced on board, including being inverted under the assumption of a Milne-Eddington atmosphere, although simpler reduction methods are also available on board. SO/PHI is composed of two telescopes; one, the Full Disc Telescope (FDT), covers the full solar disc at all phases of the orbit, while the other, the High Resolution Telescope (HRT), can resolve structures as small as 200km on the Sun at closest perihelion. The high heat load generated through proximity to the Sun is greatly reduced by the multilayer-coated entrance windows to the two telescopes that allow less than 4% of the total sunlight to enter the instrument, most of it in a narrow wavelength band around the chosen spectral line., Comment: 36 pages, 41 figures
Published: 2019
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19. First observations of speed of light tracks by a fluorescence detector looking down on the atmosphere

Author: Abdellaoui, G., Abe, S., Adams Jr., J. H., Ahriche, A., Allard, D., Allen, L., Alonso, G., Anchordoqui, L., Anzalone, A., Arai, Y., Asano, K., Attallah, R., Attoui, H., Pernas, M. Ave, Bacholle, S., Bakiri, M., Baragatti, P., Barrillon, P., Bartocci, S., Bayer, J., Beldjilali, B., Belenguer, T., Belkhalfa, N., Bellotti, R., Belov, A., Belov, K., Benmessai, K., Bertaina, M., Biermann, P. L., Biktemerova, S., Bisconti, F., Blanc, N., Błȩcki, J., Blin-Bondil, S., Bobik, P., Bogomilov, M., Bozzo, E., Bruno, A., Caballero, K. S., Cafagna, F., Campana, D., Capdevielle, J-N., Capel, F., Caramete, A., Caramete, L., Carlson, P., Caruso, R., Casolino, M., Cassardo, C., Castellina, A., Catalano, C. Catalano O., Cellino, A., Chikawa, M., Chiritoi, G., Christl, M. J., Connaughton, V., Conti, L., Cordero, G., Cotto, G., Crawford, H. J., Cremonini, R., Csorna, S., Cummings, A., Dagoret-Campagne, S., De Donato, C., de la Taille, C., De Santis, C., del Peral, L., Di Martino, M., Damian, A. Diaz, Djemil, T., Dutan, I., Ebersoldt, A., Ebisuzaki, T., Engel, R., Eser, J., Fenu, F., Fernández-González, S., Fernández-Soriano, J., Ferrarese, S., Flamini, M., Fornaro, C., Fouka, M., Franceschi, A., Franchini, S., Fuglesang, C., Fujii, T., Fujimoto, J., Fukushima, M., Galeotti, P., García-Ortega, E., Garipov, G., Gascón, E., Genci, J., Giraudo, G., Alvarado, C. González, Gorodetzky, P., Greg, R., Guarino, F., Guzmán, A., Hachisu, Y., Haiduc, M., Harlov, B., Haungs, A., Carretero, J. Hernández, Cruz, W. Hidber, Ikeda, D., Inoue, N., Inoue, S., Isgrò, F., Itow, Y., Jammer, T., Jeong, S., Joven, E., Judd, E. G., Jung, A., Jochum, J., Kajino, F., Kajino, T., Kalli, S., Kaneko, I., Karadzhov, Y., Karczmarczyk, J., Katahira, K., Kawai, K., Kawasaki, Y., Kedadra, A., Khales, H., Khrenov, B. A., Kim, Jeong-Sook, Kim, Soon-Wook, Kleifges, M., Klimov, P. A., Kolev, D., Krantz, H., Kreykenbohm, I., Kudela, K., Kurihara, Y., Kusenko, A., Kuznetsov, E., La Barbera, A., Lachaud, C., Lahmar, H., Lakhdari, F., Larson, R., Larsson, O., Lee, J., Licandro, J., Campano, L. López, Maccarone, M. C., Mackovjak, S., Mahdi, M., Maravilla, D., Marcelli, L., Marcos, J. L., Marini, A., Marszał, W., Martens, K., Martín, Y., Martinez, O., Martucci, M., Masciantonio, G., Mase, K., Mastafa, M., Matev, R., Matthews, J. N., Mebarki, N., Medina-Tanco, G., Mendoza, M. A., Menshikov, A., Merino, A., Meseguer, J., Meyer, S. S., Mimouni, J., Miyamoto, H., Mizumoto, Y., Monaco, A., Ríos, J. A. Morales de los, Nagataki, C. Moretto S., Naitamor, S., Napolitano, T., Naslund, W., Nava, R., Neronov, A., Nomoto, K., Nonaka, T., Ogawa, T., Ogio, S., Ohmori, H., Olinto, A. V., Orleański, P., Osteria, G., Pagliaro, A., Painter, W., Panasyuk, M. I., Panico, B., Pasqualino, G., Parizot, E., Park, I. H., Pastircak, B., Patzak, T., Paul, T., Pérez-Grande, I., Perfetto, F., Peter, T., Picozza, P., Pindado, S., Piotrowski, L. W., Piraino, S., Placidi, L., Plebaniak, Z., Pliego, S., Pollini, A., Polonski, Z., Popescu, E. M., Prat, P., Prévôt, G., Prieto, H., Puehlhofer, G., Putis, M., Rabanal, J., Radu, A. A., Reyes, M., Rezazadeh, M., Ricci, M., Frías, M. D. Rodríguez, Rodencal, M., Ronga, F., Roudil, G., Rusinov, I., Rybczyński, M., Sabau, M. D., Cano, G. Sáez, Sagawa, H., Sahnoune, Z., Saito, A., Sakaki, N., Salazar, H., Balanzar, J. C. Sanchez, Sánchez, J. L., Santangelo, A., Sanz-Andrés, A., Palomino, M. Sanz, Saprykin, O., Sarazin, F., Sato, M., Schanz, T., Schieler, H., Scotti, V., Selmane, S., Semikoz, D., Serra, M., Sharakin, S., Shimizu, H. M., Shinozaki, K., Shirahama, T., Spataro, B., Stan, I., Sugiyama, T., Supanitsky, D., Suzuki, M., Szabelska, B., Szabelski, J., Tajima, N., Tajima, T., Takahashi, Y., Takami, H., Takeda, M., Takizawa, Y., Talai, M. C., Tenzer, C., Thomas, S. B., Tibolla, O., Tkachev, L., Tokuno, H., Tomida, T., Tone, N., Toscano, S., Traïche, M., Tsenov, R., Tsunesada, Y., Tsuno, K., Tubbs, J., Turriziani, S., Uchihori, Y., Vaduvescu, O., Valdés-Galicia, J. F., Vallania, P., Vankova, G., Vigorito, C., Villaseñor, L., Vlcek, B., von Ballmoos, P., Vrabel, M., Wada, S., Watanabe, J., Watts Jr., J., Weber, M., Muñoz, R. Weigand, Weindl, A., Wiencke, L., Wille, M., Wilms, J., Włodarczyk, Z., Yamamoto, T., Yang, J., Yano, H., Yashin, I. V., Yonetoku, D., Yoshida, S., Young, R., Zgura, I. S, Zotov, M. Yu., and Marchi, A. Zuccaro
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: EUSO-Balloon is a pathfinder mission for the Extreme Universe Space Observatory onboard the Japanese Experiment Module (JEM-EUSO). It was launched on the moonless night of the 25$^{th}$ of August 2014 from Timmins, Canada. The flight ended successfully after maintaining the target altitude of 38 km for five hours. One part of the mission was a 2.5 hour underflight using a helicopter equipped with three UV light sources (LED, xenon flasher and laser) to perform an inflight calibration and examine the detectors capability to measure tracks moving at the speed of light. We describe the helicopter laser system and details of the underflight as well as how the laser tracks were recorded and found in the data. These are the first recorded laser tracks measured from a fluorescence detector looking down on the atmosphere. Finally, we present a first reconstruction of the direction of the laser tracks relative to the detector., Comment: 18 pages, 14 figures
Published: 2018
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20. Challenging local realism with human choices

Author: The BIG Bell Test Collaboration, Abellán, C., Acín, A., Alarcón, A., Alibart, O., Andersen, C. K., Andreoli, F., Beckert, A., Beduini, F. A., Bendersky, A., Bentivegna, M., Bierhorst, P., Burchardt, D., Cabello, A., Cariñe, J., Carrasco, S., Carvacho, G., Cavalcanti, D., Chaves, R., Cortés-Vega, J., Cuevas, A., Delgado, A., de Riedmatten, H., Eichler, C., Farrera, P., Fuenzalida, J., García-Matos, M., Garthoff, R., Gasparinetti, S., Gerrits, T., Jouneghani, F. Ghafari, Glancy, S., Gómez, E. S., González, P., Guan, J. -Y., Handsteiner, J., Heinsoo, J., Heinze, G., Hirschmann, A., Jiménez, O., Kaiser, F., Knill, E., Knoll, L. T., Krinner, S., Kurpiers, P., Larotonda, M. A., Larsson, J. -Å., Lenhard, A., Li, H., Li, M. -H., Lima, G., Liu, B., Liu, Y., Grande, I. H. López, Lunghi, T., Ma, X., Magaña-Loaiza, O. S., Magnard, P., Magnoni, A., Martí-Prieto, M., Martínez, D., Mataloni, P., Mattar, A., Mazzera, M., Mirin, R. P., Mitchell, M. W., Nam, S., Oppliger, M., Pan, J. -W., Patel, R. B., Pryde, G. J., Rauch, D., Redeker, K., Rieländer, D., Ringbauer, M., Roberson, T., Rosenfeld, W., Salathé, Y., Santodonato, L., Sauder, G., Scheidl, T., Schmiegelow, C. T., Sciarrino, F., Seri, A., Shalm, L. K., Shi, S. -C., Slussarenko, S., Stevens, M. J., Tanzilli, S., Toledo, F., Tura, J., Ursin, R., Vergyris, P., Verma, V. B., Walter, T., Wallraff, A., Wang, Z., Weinfurter, H., Weston, M. M., White, A. G., Wu, C., Xavier, G. B., You, L., Yuan, X., Zeilinger, A., Zhang, Q., Zhang, W., and Zhong, J.
Subjects: Quantum Physics
Abstract: A Bell test is a randomized trial that compares experimental observations against the philosophical worldview of local realism. A Bell test requires spatially distributed entanglement, fast and high-efficiency detection and unpredictable measurement settings. Although technology can satisfy the first two of these requirements, the use of physical devices to choose settings in a Bell test involves making assumptions about the physics that one aims to test. Bell himself noted this weakness in using physical setting choices and argued that human `free will' could be used rigorously to ensure unpredictability in Bell tests. Here we report a set of local-realism tests using human choices, which avoids assumptions about predictability in physics. We recruited about 100,000 human participants to play an online video game that incentivizes fast, sustained input of unpredictable selections and illustrates Bell-test methodology. The participants generated 97,347,490 binary choices, which were directed via a scalable web platform to 12 laboratories on five continents, where 13 experiments tested local realism using photons, single atoms, atomic ensembles, and superconducting devices. Over a 12-hour period on 30 November 2016, participants worldwide provided a sustained data flow of over 1,000 bits per second to the experiments, which used different human-generated data to choose each measurement setting. The observed correlations strongly contradict local realism and other realistic positions in bipartite and tripartite scenarios. Project outcomes include closing the `freedom-of-choice loophole' (the possibility that the setting choices are influenced by `hidden variables' to correlate with the particle properties), the utilization of video-game methods for rapid collection of human generated randomness, and the use of networking techniques for global participation in experimental science., Comment: This version includes minor changes resulting from reviewer and editorial input. Abstract shortened to fit within arXiv limits
Published: 2018
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21. The second flight of the SUNRISE balloon-borne solar observatory: overview of instrument updates, the flight, the data and first results

Author: Solanki, S. K., Riethmüller, T. L., Barthol, P., Danilovic, S., Deutsch, W., Doerr, H. P., Feller, A., Gandorfer, A., Germerott, D., Gizon, L., Grauf, B., Heerlein, K., Hirzberger, J., Kolleck, M., Lagg, A., Meller, R., Tomasch, G., van Noort, M., Rodríguez, J. Blanco, Blesa, J. L. Gasent, Jiménez, M. Balaguer, Iniesta, J. C. Del Toro, Jiménez, A. C. López, Suárez, D. Orozco, Berkefeld, T., Halbgewachs, C., Schmidt, W., Álvarez-Herrero, A., Sabau-Graziati, L., Grande, I. Pérez, Pillet, V. Martínez, Card, G., Centeno, R., Knölker, M., and Lecinski, A.
Subjects: Astrophysics - Solar and Stellar Astrophysics
Abstract: The SUNRISE balloon-borne solar observatory, consisting of a 1~m aperture telescope that provided a stabilized image to a UV filter imager and an imaging vector polarimeter, carried out its second science flight in June 2013. It provided observations of parts of active regions at high spatial resolution, including the first high-resolution images in the Mg~{\sc ii}~k line. The obtained data are of very high quality, with the best UV images reaching the diffraction limit of the telescope at 3000~\AA\ after Multi-Frame Blind Deconvolution reconstruction accounting for phase-diversity information. Here a brief update is given of the instruments and the data reduction techniques, which includes an inversion of the polarimetric data. Mainly those aspects that evolved compared with the first flight are described. A tabular overview of the observations is given. In addition, an example time series of a part of the emerging active region NOAA AR~11768 observed relatively close to disk centre is described and discussed in some detail. The observations cover the pores in the trailing polarity of the active region, as well as the polarity inversion line where flux emergence was ongoing and a small flare-like brightening occurred in the course of the time series. The pores are found to contain magnetic field strengths ranging up to 2500~G and, while large pores are clearly darker and cooler than the quiet Sun in all layers of the photosphere, the temperature and brightness of small pores approach or even exceed those of the quiet Sun in the upper photosphere., Comment: Accepted for publication in The Astrophysical Journal
Published: 2017
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22. POR QUE OS ESTUDANTES DE MEDICINA DEVEM ESTUDAR FILOSOFIA?

Author: MASSINHAN, B., primary, MERLIN, M. A. R., additional, MERLOS, F., additional, PROSDOCIMO, N. S. N., additional, MERLOS, G. C., additional, GRANDE, I. G., additional, and STREBE, B., additional
Published: 2022
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23. The mediating role of reflective functioning in the association between childhood trauma and suicide attempt

Author: Andreo-Jover, J., primary, Curto Ramos, J., additional, Bobes, J., additional, Bravo-Ortiz, M., additional, Cebria, A.I., additional, Crespo-Facorro, B., additional, De la Torre-Luque, A., additional, Díaz-Marsa, M., additional, Fernández-Rodrigues, V., additional, Garrido-Torres, N., additional, Grande, I., additional, López Peña, M.P., additional, Pemau, A., additional, Roberto, N., additional, Ruiz-Veguilla, M., additional, Saiz, P., additional, Rodríguez-Vega, B., additional, Pérez-Sola, V., additional, Palao-Tarrero, A., additional, Vicente, L., additional, Velasco, M., additional, Orgaz, B., additional, García, D., additional, Vieta, E., additional, Vázquez, M., additional, Bracco, L., additional, Gómez-Vallejo, S., additional, Díaz, C., additional, Palao, D.J., additional, Comendador, L., additional, Punti, J., additional, Muñoz, M.T., additional, García- Ramos, A., additional, Ayad-Ahmed, W., additional, Diaz-Carracedo, P., additional, Ayuso-Mateos, J.L., additional, Jimenez-Treviño, L., additional, Bobes-Bascarán, M.T., additional, Seijo-Zazo, E., additional, Fernandez-Fernandez, J., additional, Garcia-Fernandez, A., additional, Canal-Rivero, M., additional, Rider, J., additional, Reguera, P., additional, Puertas, M., additional, García-Ligero, E., additional, Tur, N., additional, Navas, M., additional, Saiz-Gonzalez, D., additional, and Carrasco, J.L., additional
Published: 2024
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24. Prediction models for suicidal behaviour in a cohort of Spanish suicide attempters

Author: Herrero, N. Roberto, primary, Prisco, M., additional, Oliva, V., additional, Pérez-Solà, V., additional, Elices, M., additional, Toll-Privat, A., additional, Bobes, J., additional, López-Peña, P., additional, Ruiz-Veguilla, M., additional, Ángela, P., additional, Annabel, C., additional, De la Torre-Luque, A., additional, Díaz-Marsà, M., additional, and Grande, I., additional
Published: 2024
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25. The diverse meteorology of Jezero crater over the first 250 sols of Perseverance on Mars

Author: Ministerio de Economía y Competitividad (España), Ministerio de Ciencia, Innovación y Universidades (España), Ministerio de Ciencia e Innovación (España), Instituto Nacional de Técnica Aeroespacial (España), European Commission, National Aeronautics and Space Administration (US), NASA Jet Propulsion Laboratory, California Institute of Technology, Rodriguez-Manfredi, J. A. [0000-0003-0461-9815], Torre Juarez, Manuel de la [0000-0003-1393-5297], Sánchez-Lavega, A. [0000-0001-7234-7634], Hueso, R. [0000-0003-0169-123X], Martinez, G. [0000-0001-5885-236X], Lemmon, M. T. [0000-0002-4504-5136], Newman, C. E. [0000-0001-9990-8817], Munguira, A. [0000-0002-1677-6327], Jaakonaho, I. [0000-0001-7343-5556], Viudez-Moreiras, D. [0000-0001-8442-3788], Ramos, M. Ángeles [0000-0003-3648-6818], Saiz-Lopez, A. [0000-0002-0060-1581], Lepinette, A. [0000-0002-5213-3521], Sullivan, R. J. [0000-0003-4191-598X], Apestigue, V. [0000-0002-4349-8019], Río Gaztelurrutia, Teresa del [0000-0001-8552-226X], Murdoch, N. [0000-0002-9701-4075], Arruego, I. [0000-0001-9705-9743], Banfield, D. [0000-0003-2664-0164], Brown, A. J. [0000-0002-9352-6989], Ceballos, J. [0000-0002-6727-1062], Dominguez-Pumar, M. [0000-0001-5439-7953], Espejo, S. [0000-0003-2609-2663], Fischer, E. [0000-0002-2098-5295], Guzewich, S. D. [0000-0003-1149-7385], Makinen, T. [0000-0001-9489-8154], Martin, C. [0000-0002-8898-4061], Molina, A. [0000-0002-5038-2022], Mora-Sotomayor, L. [0000-0002-8209-1190], Navarro, S. [0000-0001-8606-7799], Perez-Grande, I. [0000-0002-7145-2835], Romero, C. [0000-0001-5442-2581], Rodríguez-Manfredi, José Antonio, Torre Juarez, Manuel de la, Sánchez-Lavega, A., Hueso, R., Martínez, G., Lemmon, M. T., Newman, C. E., Munguira, A., Hieta, M., Tamppari, L. K., Polkko, J., Toledo, D., Sebastian, E., Smith, M. D., Jaakonaho, I., Genzer, M., Vicente-Retortillo, A. de, Viúdez-Moreiras, Daniel, Ramos, M. Ángeles, Saiz-Lopez, A., Lepinette, A., Wolff, M., Sullivan, R. J., Gómez-Elvira, Javier, Apestigue, V., Conrad, P. G., Río Gaztelurrutia, Teresa del, Murdoch, N., Arruego, I., Banfield, D., Boland, J., Brown, A. J., Ceballos, J., Dominguez-Pumar, M., Espejo, S., Fairén, A. G., Ferrandiz, R., Fischer, E., García-Villadangos, Miriam, Gimenez, S., Gomez-Gomez, F., Guzewich, S. D., Harri, A. M., Jimenez, J. J., Jimenez, V., Makinen, T., Marin, M., Martín, C., Martin-Soler, J., Molina, A., Mora-Sotomayor, L., Navarro, S., Peinado, V., Pérez-Grande, I., Pla-Garcia, J., Postigo, M., Prieto-Ballesteros, Olga, Rafkin, Scot C. R., Richardson, M. I., Romeral, J., Romero, C., Savijärvi, H., Schofield, J. T., Torres, J., Urqui, R., Zurita, S., Ministerio de Economía y Competitividad (España), Ministerio de Ciencia, Innovación y Universidades (España), Ministerio de Ciencia e Innovación (España), Instituto Nacional de Técnica Aeroespacial (España), European Commission, National Aeronautics and Space Administration (US), NASA Jet Propulsion Laboratory, California Institute of Technology, Rodriguez-Manfredi, J. A. [0000-0003-0461-9815], Torre Juarez, Manuel de la [0000-0003-1393-5297], Sánchez-Lavega, A. [0000-0001-7234-7634], Hueso, R. [0000-0003-0169-123X], Martinez, G. [0000-0001-5885-236X], Lemmon, M. T. [0000-0002-4504-5136], Newman, C. E. [0000-0001-9990-8817], Munguira, A. [0000-0002-1677-6327], Jaakonaho, I. [0000-0001-7343-5556], Viudez-Moreiras, D. [0000-0001-8442-3788], Ramos, M. Ángeles [0000-0003-3648-6818], Saiz-Lopez, A. [0000-0002-0060-1581], Lepinette, A. [0000-0002-5213-3521], Sullivan, R. J. [0000-0003-4191-598X], Apestigue, V. [0000-0002-4349-8019], Río Gaztelurrutia, Teresa del [0000-0001-8552-226X], Murdoch, N. [0000-0002-9701-4075], Arruego, I. [0000-0001-9705-9743], Banfield, D. [0000-0003-2664-0164], Brown, A. J. [0000-0002-9352-6989], Ceballos, J. [0000-0002-6727-1062], Dominguez-Pumar, M. [0000-0001-5439-7953], Espejo, S. [0000-0003-2609-2663], Fischer, E. [0000-0002-2098-5295], Guzewich, S. D. [0000-0003-1149-7385], Makinen, T. [0000-0001-9489-8154], Martin, C. [0000-0002-8898-4061], Molina, A. [0000-0002-5038-2022], Mora-Sotomayor, L. [0000-0002-8209-1190], Navarro, S. [0000-0001-8606-7799], Perez-Grande, I. [0000-0002-7145-2835], Romero, C. [0000-0001-5442-2581], Rodríguez-Manfredi, José Antonio, Torre Juarez, Manuel de la, Sánchez-Lavega, A., Hueso, R., Martínez, G., Lemmon, M. T., Newman, C. E., Munguira, A., Hieta, M., Tamppari, L. K., Polkko, J., Toledo, D., Sebastian, E., Smith, M. D., Jaakonaho, I., Genzer, M., Vicente-Retortillo, A. de, Viúdez-Moreiras, Daniel, Ramos, M. Ángeles, Saiz-Lopez, A., Lepinette, A., Wolff, M., Sullivan, R. J., Gómez-Elvira, Javier, Apestigue, V., Conrad, P. G., Río Gaztelurrutia, Teresa del, Murdoch, N., Arruego, I., Banfield, D., Boland, J., Brown, A. J., Ceballos, J., Dominguez-Pumar, M., Espejo, S., Fairén, A. G., Ferrandiz, R., Fischer, E., García-Villadangos, Miriam, Gimenez, S., Gomez-Gomez, F., Guzewich, S. D., Harri, A. M., Jimenez, J. J., Jimenez, V., Makinen, T., Marin, M., Martín, C., Martin-Soler, J., Molina, A., Mora-Sotomayor, L., Navarro, S., Peinado, V., Pérez-Grande, I., Pla-Garcia, J., Postigo, M., Prieto-Ballesteros, Olga, Rafkin, Scot C. R., Richardson, M. I., Romeral, J., Romero, C., Savijärvi, H., Schofield, J. T., Torres, J., Urqui, R., and Zurita, S.
Abstract: NASA’s Perseverance rover’s Mars Environmental Dynamics Analyzer is collecting data at Jezero crater, characterizing the physical processes in the lowest layer of the Martian atmosphere. Here we present measurements from the instrument’s first 250 sols of operation, revealing a spatially and temporally variable meteorology at Jezero. We find that temperature measurements at four heights capture the response of the atmospheric surface layer to multiple phenomena. We observe the transition from a stable night-time thermal inversion to a daytime, highly turbulent convective regime, with large vertical thermal gradients. Measurement of multiple daily optical depths suggests aerosol concentrations are higher in the morning than in the afternoon. Measured wind patterns are driven mainly by local topography, with a small contribution from regional winds. Daily and seasonal variability of relative humidity shows a complex hydrologic cycle. These observations suggest that changes in some local surface properties, such as surface albedo and thermal inertia, play an influential role. On a larger scale, surface pressure measurements show typical signatures of gravity waves and baroclinic eddies in a part of the seasonal cycle previously characterized as low wave activity. These observations, both combined and simultaneous, unveil the diversity of processes driving change on today’s Martian surface at Jezero crater.
Published: 2023

26. Ultra-violet imaging of the night-time earth by EUSO-Balloon towards space-based ultra-high energy cosmic ray observations

Author: Abdellaoui, G., Abe, S., Adams, J.H., Jr., Ahriche, A., Allard, D., Allen, L., Alonso, G., Anchordoqui, L., Anzalone, A., Arai, Y., Asano, K., Attallah, R., Attoui, H., Ave Pernas, M., Bacholle, S., Bakiri, M., Baragatti, P., Barrillon, P., Bartocci, S., Bayer, J., Beldjilali, B., Belenguer, T., Belkhalfa, N., Bellotti, R., Belov, A., Belov, K., Benmessai, K., Bertaina, M., Biermann, P.L., Biktemerova, S., Bisconti, F., Blanc, N., Błȩcki, J., Blin-Bondil, S., Bobik, P., Bogomilov, M., Bozzo, E., Briz, S., Bruno, A., Caballero, K.S., Cafagna, F., Campana, D., Capdevielle, J-N., Capel, F., Caramete, A., Caramete, L., Carlson, P., Caruso, R., Casolino, M., Cassardo, C., Castellina, A., Catalano, C., Catalano, O., Cellino, A., Chikawa, M., Chiritoi, G., Christl, M.J., Connaughton, V., Conti, L., Cordero, G., Cotto, G., Crawford, H.J., Cremonini, R., Csorna, S., Cummings, A., Dagoret-Campagne, S., de Castro, A.J., De Donato, C., de la Taille, C., De Santis, C., del Peral, L., Di Martino, M., Diaz Damian, A., Djemil, T., Dutan, I., Ebersoldt, A., Ebisuzaki, T., Engel, R., Eser, J., Fenu, F., Fernández-González, S., Ferrarese, S., Flamini, M., Fornaro, C., Fouka, M., Franceschi, A., Franchini, S., Fuglesang, C., Fujii, T., Fujimoto, J., Fukushima, M., Galeotti, P., García-Ortega, E., Garipov, G., Gascón, E., Genci, J., Giraudo, G., González Alvarado, C., Gorodetzky, P., Greg, R., Guarino, F., Guzmán, A., Hachisu, Y., Haiduc, M., Harlov, B., Haungs, A., Hernández Carretero, J., Hidber Cruz, W., Ikeda, D., Inoue, N., Inoue, S., Isgrò, F., Itow, Y., Jammer, T., Jeong, S., Joven, E., Judd, E.G., Jung, A., Jochum, J., Kajino, F., Kajino, T., Kalli, S., Kaneko, I., Karadzhov, Y., Karczmarczyk, J., Katahira, K., Kawai, K., Kawasaki, Y., Kedadra, A., Khales, H., Khrenov, B.A., Kim, Jeong-Sook, Kim, Soon-Wook, Kleifges, M., Klimov, P.A., Kolev, D., Krantz, H., Kreykenbohm, I., Krizmanic, J.F., Kudela, K., Kurihara, Y., Kusenko, A., Kuznetsov, E., La Barbera, A., Lachaud, C., Lahmar, H., Lakhdari, F., Larsson, O., Lee, J., Licandro, J., López Campano, L., López, F., Maccarone, M.C., Mackovjak, S., Mahdi, M., Maravilla, D., Marcelli, L., Marcos, J.L., Marini, A., Marszał, W., Martens, K., Martín, Y., Martinez, O., Martucci, M., Masciantonio, G., Mase, K., Mastafa, M., Matev, R., Matthews, J.N., Mebarki, N., Medina-Tanco, G., Mendoza, M.A., Menshikov, A., Merino, A., Meseguer, J., Meyer, S.S., Mimouni, J., Miyamoto, H., Mizumoto, Y., Monaco, A., Morales de los Ríos, J.A., Moretto, C., Nagataki, S., Naitamor, S., Napolitano, T., Nava, R., Neronov, A., Nomoto, K., Nonaka, T., Ogawa, T., Ogio, S., Ohmori, H., Olinto, A.V., Orleański, P., Osteria, G., Pagliaro, A., Painter, W., Panasyuk, M.I., Panico, B., Parizot, E., Park, I.H., Pastircak, B., Patzak, T., Paul, T., Pérez-Grande, I., Perfetto, F., Peter, T., Picozza, P., Pindado, S., Piotrowski, L.W., Piraino, S., Placidi, L., Plebaniak, Z., Pliego, S., Pollini, A., Polonsky, Z., Popescu, E.M., Prat, P., Prévôt, G., Prieto, H., Puehlhofer, G., Putis, M., Rabanal, J., Radu, A.A., Reyes, M., Rezazadeh, M., Ricci, M., Rodríguez Frías, M.D., Ronga, F., Roudil, G., Rusinov, I., Rybczyński, M., Sabau, M.D., Sáez Cano, G., Sagawa, H., Sahnoune, Z., Saito, A., Sakaki, N., Salazar, H., Sanchez Balanzar, J.C., Sánchez, J.L., Santangelo, A., Sanz-Andrés, A., Sanz Palomino, M., Saprykin, O., Sarazin, F., Sato, M., Schanz, T., Schieler, H., Scotti, V., Selmane, S., Semikoz, D., Serra, M., Sharakin, S., Shimizu, H.M., Shinozaki, K., Shirahama, T., Spataro, B., Stan, I., Sugiyama, T., Supanitsky, D., Suzuki, M., Szabelska, B., Szabelski, J., Tajima, N., Tajima, T., Takahashi, Y., Takami, H., Takeda, M., Takizawa, Y., Talai, M.C., Tenzer, C., Thomas, S.B., Tibolla, O., Tkachev, L., Tokuno, H., Tomida, T., Tone, N., Toscano, S., Traïche, M., Tsenov, R., Tsunesada, Y., Tsuno, K., Tubbs, J., Turriziani, S., Uchihori, Y., Vaduvescu, O., Valdés-Galicia, J.F., Vallania, P., Vankova, G., Vigorito, C., Villaseñor, L., Vlcek, B., von Ballmoos, P., Vrabel, M., Wada, S., Watanabe, J., Watts, J., Jr., Weber, M., Weigand Muñoz, R., Weindl, A., Wiencke, L., Wille, M., Wilms, J., Włodarczyk, Z., Yamamoto, T., Yang, J., Yano, H., Yashin, I.V., Yonetoku, D., Yoshida, S., Young, R., Zgura, I.S., Zotov, M.Yu., and Zuccaro Marchi, A.
Published: 2019
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27. Behavioral addictions in bipolar disorders: A systematic review

Author: Varo, C, Murru, A, Salagre, E, Jiménez, E, Solé, B, Montejo, L, Carvalho, AF, Stubbs, B, Grande, I, Martínez-Arán, A, Vieta, E, and Reinares, M
Published: 2019
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28. Determination of the SO/PHI-HRT wavefront degradation using multiple defocused images

Author: Bailén, F.J., primary, Orozco Suárez, D., additional, Blanco Rodríguez, J., additional, del Toro Iniesta, J.C., additional, Strecker, H., additional, Moreno Vacas, A., additional, Santamarina Guerrero, P., additional, Hirzberger, J., additional, Albert, K., additional, Albelo Jorge, N., additional, Appourchaux, T., additional, Alvarez-Herrero, A., additional, Gandorfer, A., additional, Germerott, D., additional, Guerrero, L., additional, Gutierrez-Marques, P., additional, Kahil, F., additional, Kolleck, M., additional, Solanki, S.K., additional, Volkmer, R., additional, Woch, J., additional, Fiethe, B., additional, Gómez Cama, J.M., additional, Pérez-Grande, I., additional, Sanchis Kilders, E., additional, Balaguer Jiménez, M., additional, Bellot Rubio, L.R., additional, Calchetti, D., additional, Carmona, M., additional, Deutsch, W., additional, Feller, A., additional, Fernandez-Rico, G., additional, Fernández-Medina, A., additional, García Parejo, P., additional, Gasent Blesa, J.L., additional, Gizon, L., additional, Grauf, B., additional, Heerlein, K., additional, Korpi-Lagg, A., additional, Lange, T., additional, López Jiménez, A., additional, Maue, T., additional, Meller, R., additional, Michalik, H., additional, Müller, R., additional, Nakai, E., additional, Schmidt, W., additional, Schou, J., additional, Schühle, U., additional, Sinjan, J., additional, Staub, J., additional, Torralbo, I., additional, and Valori, G., additional
Published: 2023
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29. A first rapid synoptic magnetic field map using SDO/HMI andSO/PHI data

Author: Loeschl, P., primary, Valori, G., additional, Hirzberger, J., additional, Schou, J., additional, Solanki, S.K., additional, Orozco Suarez, D., additional, Albert, K., additional, Albelo Jorge, N., additional, Appourchaux, T., additional, Alvarez-Herrero, A., additional, Blanco Rodriguez, J., additional, Gandorfer, A., additional, Germerott, D., additional, Guerrero, L., additional, Gutierrez-Marques, P., additional, Kahil, F., additional, Kolleck, M., additional, del Toro Iniesta, J.C., additional, Volkmer, R., additional, Woch, J., additional, Fiethe, B., additional, Gómez Cama, J.M., additional, Perez-Grande, I., additional, Sanchis Kilders, E., additional, Balaguer Jiménez, M., additional, Bellot Rubio, L.R., additional, Calchetti, D., additional, Carmona, M., additional, Deutsch, W., additional, Feller, A., additional, Fernandez-Rico, G., additional, Fernandez-Medina, A., additional, Garcia Perejo, P., additional, Gasent Blesa, J.L., additional, Gizon, L., additional, Grauf, B., additional, Heerlein, K., additional, Korpi-Lagg, A., additional, Lange, T., additional, Lopez Jimenez, A., additional, Maue, T., additional, Meller, R., additional, Michalik, H., additional, Moreno Vacas, A., additional, Müller, R., additional, Nakai, E., additional, Schmidt, W., additional, Schühle, U., additional, Sinjan, J., additional, Staub, J., additional, Strecker, H., additional, and Torralbo, I., additional
Published: 2023
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30. Reconstruction of total solar irradiance variability as simultaneously apparent from Solar Orbiter and Solar Dynamics Observatory

Author: Yeo, K. L., primary, Krivova, N. A., additional, Solanki, S. K., additional, Hirzberger, J., additional, Orozco Suárez, D., additional, Albert, K., additional, Albelo Jorge, N., additional, Appourchaux, T., additional, Alvarez-Herrero, A., additional, Blanco Rodríguez, J., additional, Gandorfer, A., additional, Gutierrez-Marques, P., additional, Kahil, F., additional, Kolleck, M., additional, del Toro Iniesta, J. C., additional, Volkmer, R., additional, Woch, J., additional, Fiethe, B., additional, Pérez-Grande, I., additional, Sanchis Kilders, E., additional, Balaguer Jiménez, M., additional, Bellot Rubio, L. R., additional, Calchetti, D., additional, Carmona, M., additional, Feller, A., additional, Fernandez-Rico, G., additional, Fernández-Medina, A., additional, García Parejo, P., additional, Gasent Blesa, J. L., additional, Gizon, L., additional, Grauf, B., additional, Heerlein, K., additional, Korpi-Lagg, A., additional, Maue, T., additional, Meller, R., additional, Moreno Vacas, A., additional, Müller, R., additional, Nakai, E., additional, Schmidt, W., additional, Schou, J., additional, Sinjan, J., additional, Staub, J., additional, Strecker, H., additional, Torralbo, I., additional, and Valori, G., additional
Published: 2023
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31. Intensity contrast of solar network and faculae close to the solar limb, observed from two vantage points

Author: Albert, K., primary, Krivova, N. A., additional, Hirzberger, J., additional, Solanki, S. K., additional, Moreno Vacas, A., additional, Orozco Suárez, D., additional, Albelo Jorge, N., additional, Appourchaux, T., additional, Alvarez-Herrero, A., additional, Blanco Rodríguez, J., additional, Gandorfer, A., additional, Gutierrez-Marques, P., additional, Kahil, F., additional, Kolleck, M., additional, Volkmer, R., additional, del Toro Iniesta, J. C., additional, Woch, J., additional, Fiethe, B., additional, Pérez-Grande, I., additional, Sanchis Kilders, E., additional, Balaguer Jiménez, M., additional, Bellot Rubio, L. R., additional, Calchetti, D., additional, Carmona, M., additional, Deutsch, W., additional, Feller, A., additional, Fernandez-Rico, G., additional, Fernández-Medina, A., additional, García Parejo, P., additional, Gasent Blesa, J. L., additional, Gizon, L., additional, Grauf, B., additional, Heerlein, K., additional, Korpi-Lagg, A., additional, Lange, T., additional, López Jiménez, A., additional, Maue, T., additional, Meller, R., additional, Müller, R., additional, Nakai, E., additional, Schmidt, W., additional, Schou, J., additional, Sinjan, J., additional, Staub, J., additional, Strecker, H., additional, Torralbo, I., additional, and Valori, G., additional
Published: 2023
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32. Coronal voids and their magnetic nature

Author: Nölke, J. D., primary, Solanki, S. K., additional, Hirzberger, J., additional, Peter, H., additional, Chitta, L. P., additional, Kahil, F., additional, Valori, G., additional, Wiegelmann, T., additional, Orozco Suárez, D., additional, Albert, K., additional, Albelo Jorge, N., additional, Appourchaux, T., additional, Alvarez-Herrero, A., additional, Blanco Rodríguez, J., additional, Gandorfer, A., additional, Germerott, D., additional, Guerrero, L., additional, Gutierrez-Marques, P., additional, Kolleck, M., additional, del Toro Iniesta, J. C., additional, Volkmer, R., additional, Woch, J., additional, Fiethe, B., additional, Gómez Cama, J. M., additional, Pérez-Grande, I., additional, Sanchis Kilders, E., additional, Balaguer Jiménez, M., additional, Bellot Rubio, L. R., additional, Calchetti, D., additional, Carmona, M., additional, Deutsch, W., additional, Feller, A., additional, Fernandez-Rico, G., additional, Fernández-Medina, A., additional, García Parejo, P., additional, Gasent Blesa, J. L., additional, Gizon, L., additional, Grauf, B., additional, Heerlein, K., additional, Korpi-Lagg, A., additional, Lange, T., additional, López Jiménez, A., additional, Maue, T., additional, Meller, R., additional, Moreno Vacas, A., additional, Müller, R., additional, Nakai, E., additional, Schmidt, W., additional, Schou, J., additional, Schühle, U., additional, Sinjan, J., additional, Staub, J., additional, Strecker, H., additional, Torralbo, I., additional, Berghmans, D., additional, Kraaikamp, E., additional, Rodriguez, L., additional, Verbeeck, C., additional, Zhukov, A. N., additional, Auchere, F., additional, Buchlin, E., additional, Parenti, S., additional, Janvier, M., additional, Barczynski, K., additional, Harra, L., additional, Schwanitz, C., additional, Aznar Cuadrado, R., additional, Mandal, S., additional, Teriaca, L., additional, Long, D., additional, and Smith, P., additional
Published: 2023
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33. Use of the Functioning Assessment Short Test (FAST) in defining functional recovery in bipolar I disorder. Post-hoc analyses of long-term studies of aripiprazole once monthly as maintenance treatment

Author: Madera J, Such P, Zhang P, Baker RA, and Grande I
Subjects: Bipolar disorder, aripiprazole, long-acting injectable, maintenance, functioning, recovery, Neurosciences. Biological psychiatry. Neuropsychiatry, RC321-571, Neurology. Diseases of the nervous system, RC346-429
Abstract: Jessica Madera,1 Pedro Such,2 Peter Zhang,1 Ross A Baker,1 Iria Grande31Medical Affairs, Otsuka Pharmaceutical Development and Commercialization Inc, Princeton, NJ, USA; 2Medical Affairs, H. Lundbeck A/S, Valby, Denmark; 3Bipolar and Depression Disorders Unit, Hospital Clinic, Institute of Neurosciences, University of Barcelona, IDIBAPS, CIBERSAM, Barcelona, Catalonia, SpainPurpose: There is growing agreement that definitions of “recovery” in bipolar-I disorder (BP-I) should include functional outcomes beyond sustained symptomatic remission. In this post-hoc analysis, we assessed functional recovery rates according to the validated Functioning Assessment Short Test (FAST) in participants with BP-I after 52 weeks of maintenance treatment with aripiprazole once monthly (AOM).Patients and methods: Rates of functional recovery with AOM 400 were investigated in two 52-week studies. NCT01567527 was a placebo-controlled, double-blind, randomized-withdrawal study and NCT01710709 was an open-label study. Functional recovery, assessed at the end of the respective maintenance phases, was defined as a total FAST score of ≤11 for 8 consecutive weeks.Results: Post-hoc analyses included 229 patients from the randomized-withdrawal study (AOM 400 n=116; placebo n=113). The open-label study included 402 patients (including 321 de novo patients and 81 rollover patients who had completed the randomized-withdrawal study). In the randomized-withdrawal study, functional recovery was achieved by 30.2% (n=35) of the AOM 400 group compared with 24.8% (n=28) in the placebo group. The difference was not statistically significant (p=0.39). In the open-label study, 36% (n=116) of de novo patients and 43% (n=35) of rollover patients had functionally recovered after 52 weeks of AOM 400 treatment.Conclusion: These data highlight the utility of a sustained FAST total score of ≤11 as a definition of recovery and emphasize the possibility of achieving this ambitious treatment goal with effective long-term treatment.Keywords: bipolar disorder, aripiprazole, long-acting injectable, maintenance, functioning, recovery
Published: 2019

34. EUSO-TA – First results from a ground-based EUSO telescope

Author: Abdellaoui, G., Abe, S., Adams, J.H., Jr., Ahriche, A., Allard, D., Allen, L., Alonso, G., Anchordoqui, L., Anzalone, A., Arai, Y., Asano, K., Attallah, R., Attoui, H., Ave Pernas, M., Bacholle, S., Bakiri, M., Baragatti, P., Barrillon, P., Bartocci, S., Bayer, J., Beldjilali, B., Belenguer, T., Belkhalfa, N., Bellotti, R., Belov, A., Belov, K., Belz, J.W., Benmessai, K., Bertaina, M., Biermann, P.L., Biktemerova, S., Bisconti, F., Blanc, N., Blecki, J., Blin-Bondil, S., Bobik, P., Bogomilov, M., Bozzo, E., Bruno, A., Caballero, K.S., Cafagna, F., Campana, D., Capdevielle, J-N., Capel, F., Caramete, A., Caramete, L., Carlson, P., Caruso, R., Casolino, M., Cassardo, C., Castellina, A., Catalano, O., Cellino, A., Chikawa, M., Chiritoi, G., Christl, M.J., Connaughton, V., Conti, L., Cordero, G., Cotto, G., Crawford, H.J., Cremonini, R., Csorna, S., Cummings, A., Dagoret-Campagne, S., De Donato, C., de la Taille, C., De Santis, C., del Peral, L., Di Martino, M., Djemil, T., Dutan, I., Ebersoldt, A., Ebisuzaki, T., Engel, R., Eser, J., Fenu, F., Fernández-González, S., Fernández-Soriano, J., Ferrarese, S., Flamini, M., Fornaro, C., Fouka, M., Franceschi, A., Franchini, S., Fuglesang, C., Fujii, T., Fujimoto, J., Fukushima, M., Galeotti, P., García-Ortega, E., Garipov, G., Gascón, E., Genci, J., Giraudo, G., González Alvarado, C., Gorodetzky, P., Greg, R., Guarino, F., Guzmán, A., Hachisu, Y., Haiduc, M., Harlov, B., Haungs, A., Hernández Carretero, J., Hidber Cruz, W., Ikeda, D., Inoue, N., Inoue, S., Isgrò, F., Itow, Y., Jammer, T., Jeong, S., Joven, E., Judd, E.G., Jung, A., Jochum, J., Kajino, F., Kajino, T., Kalli, S., Kaneko, I., Karadzhov, Y., Karczmarczyk, J., Katahira, K., Kawai, K., Kawasaki, Y., Kedadra, A., Khales, H., Khrenov, B.A., Kim, Jeong-Sook, Kim, Soon-Wook, Kleifges, M., Klimov, P.A., Kolev, D., Krantz, H., Kreykenbohm, I., Kudela, K., Kurihara, Y., Kusenko, A., Kuznetsov, E., La Barbera, A., Lachaud, C., Lahmar, H., Lakhdari, F., Larsson, O., Lee, J., Licandro, J., López Campano, L., Maccarone, M.C., Mackovjak, S., Mahdi, M., Maravilla, D., Marcelli, L., Marcos, J.L., Marini, A., Marszal, W., Martens, K., Martín, Y., Martinez, O., Martucci, M., Masciantonio, G., Mase, K., Mustafa, M., Matev, R., Matthews, J.N., Mebarki, N., Medina-Tanco, G., Mendoza, M.A., Menshikov, A., Merino, A., Meseguer, J., Meyer, S.S., Mimouni, J., Miyamoto, H., Mizumoto, Y., Monaco, A., Morales de los Ríos, J.A., Nagataki, S., Naitamor, S., Napolitano, T., Nava, R., Neronov, A., Nomoto, K., Nonaka, T., Ogawa, T., Ogio, S., Ohmori, H., Olinto, A.V., Orleański, P., Osteria, G., Pagliaro, A., Painter, W., Panasyuk, M.I., Panico, B., Parizot, E., Park, I.H., Pastircak, B., Patzak, T., Paul, T., Pérez-Grande, I., Perfetto, F., Peter, T., Picozza, P., Pindado, S., Piotrowski, L.W., Piraino, S., Placidi, L., Plebaniak, Z., Pliego, S., Pollini, A., Polonski, Z., Popescu, E.M., Prat, P., Prévôt, G., Prieto, H., Puehlhofer, G., Putis, M., Rabanal, J., Radu, A.A., Reyes, M., Rezazadeh, M., Ricci, M., Rodríguez Frías, M.D., Ronga, F., Roudil, G., Rusinov, I., Rybczyński, M., Sabau, M.D., Sáez Cano, G., Sagawa, H., Sahnoune, Z., Saito, A., Sakaki, N., Salazar, H., Sanchez Balanzar, J.C., Sánchez, J.L., Santangelo, A., Sanz-Andrés, A., Sanz Palomino, M., Saprykin, O., Sarazin, F., Sato, M., Schanz, T., Schieler, H., Scotti, V., Selmane, S., Semikoz, D., Serra, M., Sharakin, S., Shimizu, H.M., Shin, H.S., Shinozaki, K., Shirahama, T., Sokolsky, P., Spataro, B., Stan, I., Sugiyama, T., Supanitsky, D., Suzuki, M., Szabelska, B., Szabelski, J., Tajima, N., Tajima, T., Takahashi, Y., Takami, H., Takeda, M., Takizawa, Y., Talai, M.C., Tameda, Y., Tenzer, C., Thomas, S.B., Thomson, G.B., Tibolla, O., Tkachev, L., Tokuno, H., Tomida, T., Tone, N., Toscano, S., Traïche, M., Tsenov, R., Tsunesada, Y., Tsuno, K., Tubbs, J., Turriziani, S., Uchihori, Y., Vaduvescu, O., Valdés-Galicia, J.F., Vallania, P., Vankova, G., Vigorito, C., Villaseñor, L., Vlcek, B., von Ballmoos, P., Vrabel, M., Wada, S., Watanabe, J., Watts, J., Jr., Weber, M., Weigand Muñoz, R., Weindl, A., Wiencke, L., Wille, M., Wilms, J., Włodarczyk, Z., Yamamoto, T., Yang, J., Yano, H., Yashin, I.V., Yonetoku, D., Yoshida, S., Young, R., Zgura, I.S., Zotov, M.Yu., and Zuccaro Marchi, A.
Published: 2018
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35. The Mars Environmental Dynamics Analyzer, MEDA. A Suite of Environmental Sensors for the Mars 2020 Mission

Author: Rodriguez-Manfredi, J. A., de la Torre Juárez, M., Alonso, A., Apéstigue, V., Arruego, I., Atienza, T., Banfield, D., Boland, J., Carrera, M. A., Castañer, L., Ceballos, J., Chen-Chen, H., Cobos, A., Conrad, P. G., Cordoba, E., del Río-Gaztelurrutia, T., de Vicente-Retortillo, A., Domínguez-Pumar, M., Espejo, S., Fairen, A. G., Fernández-Palma, A., Ferrándiz, R., Ferri, F., Fischer, E., García-Manchado, A., García-Villadangos, M., Genzer, M., Giménez, S., Gómez-Elvira, J., Gómez, F., Guzewich, S. D., Harri, A.-M., Hernández, C. D., Hieta, M., Hueso, R., Jaakonaho, I., Jiménez, J. J., Jiménez, V., Larman, A., Leiter, R., Lepinette, A., Lemmon, M. T., López, G., Madsen, S. N., Mäkinen, T., Marín, M., Martín-Soler, J., Martínez, G., Molina, A., Mora-Sotomayor, L., Moreno-Álvarez, J. F., Navarro, S., Newman, C. E., Ortega, C., Parrondo, M. C., Peinado, V., Peña, A., Pérez-Grande, I., Pérez-Hoyos, S., Pla-García, J., Polkko, J., Postigo, M., Prieto-Ballesteros, O., Rafkin, S. C. R., Ramos, M., Richardson, M. I., Romeral, J., Romero, C., Runyon, K. D., Saiz-Lopez, A., Sánchez-Lavega, A., Sard, I., Schofield, J. T., Sebastian, E., Smith, M. D., Sullivan, R. J., Tamppari, L. K., Thompson, A. D., Toledo, D., Torrero, F., Torres, J., Urquí, R., Velasco, T., Viúdez-Moreiras, D., and Zurita, S.
Published: 2021
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36. Psychometric properties of the well-being index (WHO-5) spanish version in a sample of euthymic patients with bipolar disorder

Author: Bonnín, C.M., Yatham, L.N., Michalak, E.E., Martínez-Arán, A., Dhanoa, T., Torres, I., Santos-Pascual, C., Valls, E., Carvalho, A.F., Sánchez-Moreno, J., Valentí, M., Grande, I., Hidalgo-Mazzei, D., Vieta, E., and Reinares, M.
Published: 2018
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37. Stereoscopic disambiguation of vector magnetograms: First applications to SO/PHI-HRT data

Author: Valori, G., primary, Calchetti, D., additional, Moreno Vacas, A., additional, Pariat, É., additional, Solanki, S. K., additional, Löschl, P., additional, Hirzberger, J., additional, Parenti, S., additional, Albert, K., additional, Albelo Jorge, N., additional, Álvarez-Herrero, A., additional, Appourchaux, T., additional, Bellot Rubio, L. R., additional, Blanco Rodríguez, J., additional, Campos-Jara, A., additional, Feller, A., additional, Gandorfer, A., additional, García Parejo, P., additional, Germerott, D., additional, Gizon, L., additional, Gómez Cama, J. M., additional, Guerrero, L., additional, Gutierrez-Marques, P., additional, Kahil, F., additional, Kolleck, M., additional, Korpi-Lagg, A., additional, Orozco Suárez, D., additional, Pérez-Grande, I., additional, Sanchis Kilders, E., additional, Schou, J., additional, Schühle, U., additional, Sinjan, J., additional, Staub, J., additional, Strecker, H., additional, del Toro Iniesta, J. C., additional, Volkmer, R., additional, and Woch, J., additional
Published: 2023
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38. Automated mood disorder symptoms monitoring from multivariate time-series sensory data: Getting the full picture beyond a single number.

Author: Corponi, Filippo, primary, Li, Bryan, additional, Anmella, Gerard, additional, Mas, Ariadna, additional, Pacchiarotti, Isabella, additional, Valentí, Marc, additional, Fullana, Iria Grande i, additional, Benabarre, Antonio, additional, Garriga, Marina, additional, Vieta, Eduard, additional, Lawrie, Stephen, additional, Whalley, Heather, additional, Hidalgo-Mazzei, Diego, additional, and Vergari, Antonio, additional
Published: 2023
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39. Treatment of neurocognitive symptoms in unipolar depression: A systematic review and future perspectives

Author: Salagre, E., Solé, B., Tomioka, Y., Fernandes, B.S., Hidalgo-Mazzei, D., Garriga, M., Jimenez, E., Sanchez-Moreno, J., Vieta, E., and Grande, I.
Published: 2017
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40. Cosmic ray oriented performance studies for the JEM-EUSO first level trigger

Author: Abdellaoui, G., Abe, S., Acheli, A., Adams, J.H., Jr., Ahmad, S., Ahriche, A., Albert, J.-N., Allard, D., Alonso, G., Anchordoqui, L., Andreev, V., Anzalone, A., Aouimeur, W., Arai, Y., Arsene, N., Asano, K., Attallah, R., Attoui, H., Ave Pernas, M., Bacholle, S., Bakiri, M., Baragatti, P., Barrillon, P., Bartocci, S., Batsch, T., Bayer, J., Bechini, R., Belenguer, T., Bellotti, R., Belov, A., Belov, K., Benadda, B., Benmessai, K., Berlind, A.A., Bertaina, M., Biermann, P.L., Biktemerova, S., Bisconti, F., Blanc, N., Błȩcki, J., Blin-Bondil, S., Bobik, P., Bogomilov, M., Bonamente, M., Boudaoud, R., Bozzo, E., Briggs, M.S., Bruno, A., Caballero, K.S., Cafagna, F., Campana, D., Capdevielle, J.-N., Capel, F., Caramete, A., Caramete, L., Carlson, P., Caruso, R., Casolino, M., Cassardo, C., Castellina, A., Castellini, G., Catalano, C., Catalano, O., Cellino, A., Chikawa, M., Chiritoi, G., Christl, M.J., Connaughton, V., Conti, L., Contino, G., Cordero, G., Cotto, G., Crawford, H.J., Cremonini, R., Csorna, S., Dagoret-Campagne, S., De Donato, C., de la Taille, C., De Santis, C., del Peral, L., Di Martino, M., Djemil, T., Djenas, S.A., Dulucq, F., Dupieux, M., Dutan, I., Ebersoldt, A., Ebisuzaki, T., Engel, R., Eser, J., Fang, K., Fenu, F., Fernández-González, S., Fernández-Soriano, J., Ferrarese, S., Finco, D., Flamini, M., Fornaro, C., Forza, R., Fouka, M., Franceschi, A., Franchini, S., Fuglesang, C., Fujimoto, J., Fukushima, M., Galeotti, P., García-Ortega, E., Garipov, G., Gascón, E., Geary, J., Gelmini, G., Genci, J., Giraudo, G., Gonchar, M., González Alvarado, C., Gorodetzky, P., Guardone, N., Guarino, F., Guehaz, R., Guzmán, A., Hachisu, Y., Haiduc, M., Harlov, B., Haungs, A., Hernández Carretero, J., Hidber, W., Higashide, K., Ikeda, D., Ikeda, H., Inoue, N., Inoue, S., Insolia, A., Isgrò, F., Itow, Y., Jammer, T., Joven, E., Judd, E.G., Jung, A., Jochum, J., Kajino, F., Kajino, T., Kalli, S., Kaneko, I., Kang, D., Kanouni, F., Karadzhov, Y., Karczmarczyk, J., Karus, M., Katahira, K., Kawai, K., Kawasaki, Y., Kedadra, A., Khales, H., Khrenov, B.A., Kim, Jeong-Sook, Kim, Soon-Wook, Kim, Sug-Whan, Kleifges, M., Klimov, P.A., Kolev, D., Kreykenbohm, I., Kudela, K., Kurihara, Y., Kusenko, A., Kuznetsov, E., Lacombe, M., Lachaud, C., Lahmar, H., Lakhdari, F., Larsson, O., Lee, J., Licandro, J., Lim, H., López Campano, L., Maccarone, M.C., Mackovjak, S., Mahdi, M., Manfrin, M., Maravilla, D., Marcelli, L., Marcos, J.L., Marini, A., Martens, K., Martín, Y., Martinez, O., Masciantonio, G., Mase, K., Matev, R., Matthews, J.N., Mebarki, N., Medina-Tanco, G., Mehrad, L., Mendoza, M.A., Merino, A., Mernik, T., Meseguer, J., Messaoud, S., Micu, O., Mignone, M., Mimouni, J., Miyamoto, H., Miyazaki, Y., Mizumoto, Y., Modestino, G., Monaco, A., Monnier-Ragaigne, D., Morales de los Ríos, J.A., Moretto, C., Morozenko, V.S., Mot, B., Murakami, T., Nadji, B., Nagano, M., Nagata, M., Nagataki, S., Nakamura, T., Napolitano, T., Naumov, D., Nava, R., Neronov, A., Nomoto, K., Nonaka, T., Ogawa, T., Ogio, S., Ohmori, H., Olinto, A.V., Orleański, P., Osteria, G., Painter, W., Panasyuk, M.I., Panico, B., Parizot, E., Park, I.H., Park, H.W., Pastircak, B., Patzak, T., Paul, T., Pennypacker, C., Pérez-Grande, I., Perfetto, F., Peter, T., Picozza, P., Pierog, T., Pindado, S., Piotrowski, L.W., Piraino, S., Placidi, L., Plebaniak, Z., Pliego, S., Pollini, A., Popescu, E.M., Prat, P., Prévôt, G., Prieto, H., Putis, M., Rabanal, J., Radu, A.A., Rahmani, M., Reardon, P., Reyes, M., Rezazadeh, M., Ricci, M., Rodríguez Frías, M.D., Ronga, F., Roth, M., Rothkaehl, H., Roudil, G., Rusinov, I., Rybczyński, M., Sabau, M.D., Sáez Cano, G., Sagawa, H., Sahnoune, Z., Saito, A., Sakaki, N., Sakata, M., Salazar, H., Sanchez, J.C., Sánchez, J.L., Santangelo, A., Santiago Crúz, L., Sanz-Andrés, A., Sanz Palomino, M., Saprykin, O., Sarazin, F., Sato, H., Sato, M., Schanz, T., Schieler, H., Scotti, V., Segreto, A., Selmane, S., Semikoz, D., Serra, M., Sharakin, S., Shibata, T., Shimizu, H.M., Shinozaki, K., Shirahama, T., Siemieniec-Oziȩbło, G., Sledd, J., Słomińska, K., Sobey, A., Stan, I., Sugiyama, T., Supanitsky, D., Suzuki, M., Szabelska, B., Szabelski, J., Tahi, H., Tajima, F., Tajima, N., Tajima, T., Takahashi, Y., Takami, H., Takeda, M., Takizawa, Y., Talai, M.C., Tenzer, C., Tibolla, O., Tkachev, L., Tokuno, H., Tomida, T., Tone, N., Toscano, S., Traïche, M., Tsenov, R., Tsunesada, Y., Tsuno, K., Tymieniecka, T., Uchihori, Y., Unger, M., Vaduvescu, O., Valdés-Galicia, J.F., Vallania, P., Vankova, G., Vigorito, C., Villaseñor, L., Vlcek, B., von Ballmoos, P., Vrabel, M., Wada, S., Watanabe, J., Watanabe, S., Watts, J., Jr., Weber, M., Weigand Muñoz, R., Weindl, A., Weiler, T.J., Wibig, T., Wiencke, L., Wille, M., Wilms, J., Włodarczyk, Z., Yamamoto, T., Yamamoto, Y., Yang, J., Yano, H., Yashin, I.V., Yonetoku, D., Yoshida, S., Young, R., Zgura, I.S., Zotov, M.Yu., and Zuccaro Marchi, A.
Published: 2017
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41. High cognitive reserve in bipolar disorders as a moderator of neurocognitive impairment

Author: Grande, I., Sanchez-Moreno, J., Sole, B., Jimenez, E., Torrent, C., Bonnin, C.M., Varo, C., Tabares-Seisdedos, R., Balanzá-Martínez, V., Valls, E., Morilla, I., Carvalho, A.F., Ayuso-Mateos, J.L., Vieta, E., and Martinez-Aran, A.
Published: 2017
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42. Wavefront error of PHI/HRT on Solar Orbiter at various heliocentric distances

Author: Kahil, F., primary, Gandorfer, A., additional, Hirzberger, J., additional, Calchetti, D., additional, Sinjan, J., additional, Valori, G., additional, Solanki, S. K., additional, Van Noort, M., additional, Albert, K., additional, Albelo Jorge, N., additional, Alvarez-Herrero, A., additional, Appourchaux, T., additional, Bellot Rubio, L. R., additional, Blanco Rodríguez, J., additional, Feller, A., additional, Fiethe, B., additional, Germerott, D., additional, Gizon, L., additional, Guerrero, L., additional, Gutierrez-Marques, P., additional, Kolleck, M., additional, Korpi-Lagg, A., additional, Michalik, H., additional, Moreno Vacas, A., additional, Orozco Suárez, D., additional, Pérez-Grande, I., additional, Sanchis Kilders, E., additional, Schou, J., additional, Schühle, U., additional, Staub, J., additional, Strecker, H., additional, del Toro Iniesta, J. C., additional, Volkmer, R., additional, and Woch, J., additional
Published: 2023
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43. Direct assessment of SDO/HMI helioseismology of active regions on the Sun’s far side using SO/PHI magnetograms

Author: Yang, D., primary, Gizon, L., additional, Barucq, H., additional, Hirzberger, J., additional, Orozco Suárez, D., additional, Albert, K., additional, Albelo Jorge, N., additional, Appourchaux, T., additional, Alvarez-Herrero, A., additional, Blanco Rodríguez, J., additional, Gandorfer, A., additional, Germerott, D., additional, Guerrero, L., additional, Gutierrez-Marques, P., additional, Kahil, F., additional, Kolleck, M., additional, Solanki, S. K., additional, del Toro Iniesta, J. C., additional, Volkmer, R., additional, Woch, J., additional, Pérez-Grande, I., additional, Sanchis Kilders, E., additional, Balaguer Jiménez, M., additional, Bellot Rubio, L. R., additional, Calchetti, D., additional, Carmona, M., additional, Deutsch, W., additional, Feller, A., additional, Fernandez-Rico, G., additional, Fernández-Medina, A., additional, García Parejo, P., additional, Gasent Blesa, J. L., additional, Grauf, B., additional, Heerlein, K., additional, Korpi-Lagg, A., additional, Lange, T., additional, López Jiménez, A., additional, Maue, T., additional, Meller, R., additional, Moreno Vacas, A., additional, Müller, R., additional, Nakai, E., additional, Schmidt, W., additional, Schou, J., additional, Schühle, U., additional, Sinjan, J., additional, Staub, J., additional, Strecker, H., additional, Torralbo, I., additional, and Valori, G., additional
Published: 2023
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44. Spectropolarimetric investigation of magnetohydrodynamic wave modes in the photosphere: First results from PHI on board Solar Orbiter

Author: Calchetti, D., primary, Stangalini, M., additional, Jafarzadeh, S., additional, Valori, G., additional, Albert, K., additional, Albelo Jorge, N., additional, Alvarez-Herrero, A., additional, Appourchaux, T., additional, Balaguer Jiménez, M., additional, Bellot Rubio, L. R., additional, Blanco Rodríguez, J., additional, Feller, A., additional, Gandorfer, A., additional, Germerott, D., additional, Gizon, L., additional, Guerrero, L., additional, Gutierrez-Marques, P., additional, Hirzberger, J., additional, Kahil, F., additional, Kolleck, M., additional, Korpi-Lagg, A., additional, Moreno Vacas, A., additional, Orozco Suárez, D., additional, Pérez-Grande, I., additional, Sanchis Kilders, E., additional, Schou, J., additional, Schühle, U., additional, Sinjan, J., additional, Solanki, S. K., additional, Staub, J., additional, Strecker, H., additional, del Toro Iniesta, J. C., additional, Volkmer, R., additional, and Woch, J., additional
Published: 2023
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45. The ratio of horizontal to vertical displacement in solar oscillations estimated from combined SO/PHI and SDO/HMI observations

Author: Schou, J., primary, Hirzberger, J., additional, Orozco Suárez, D., additional, Albert, K., additional, Albelo Jorge, N., additional, Appourchaux, T., additional, Alvarez-Herrero, A., additional, Blanco Rodríguez, J., additional, Gandorfer, A., additional, Germerott, D., additional, Guerrero, L., additional, Gutierrez-Marques, P., additional, Kahil, F., additional, Kolleck, M., additional, Solanki, S. K., additional, del Toro Iniesta, J. C., additional, Volkmer, R., additional, Woch, J., additional, Fiethe, B., additional, Pérez-Grande, I., additional, Sanchis Kilders, E., additional, Balaguer Jiménez, M., additional, Bellot Rubio, L. R., additional, Calchetti, D., additional, Carmona, M., additional, Deutsch, W., additional, Feller, A., additional, Fernandez-Rico, G., additional, Fernández-Medina, A., additional, García Parejo, P., additional, Gasent Blesa, J. L., additional, Gizon, L., additional, Grauf, B., additional, Heerlein, K., additional, Korpi-Lagg, A., additional, López Jiménez, A., additional, Maue, T., additional, Meller, R., additional, Moreno Vacas, A., additional, Müller, R., additional, Nakai, E., additional, Schmidt, W., additional, Sinjan, J., additional, Staub, J., additional, Strecker, H., additional, Torralbo, I., additional, and Valori, G., additional
Published: 2023
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46. Magnetic fields inferred by Solar Orbiter: A comparison between SO/PHI-HRT and SDO/HMI

Author: Sinjan, J., primary, Calchetti, D., additional, Hirzberger, J., additional, Kahil, F., additional, Valori, G., additional, Solanki, S. K., additional, Albert, K., additional, Albelo Jorge, N., additional, Alvarez-Herrero, A., additional, Appourchaux, T., additional, Bellot Rubio, L. R., additional, Blanco Rodríguez, J., additional, Feller, A., additional, Gandorfer, A., additional, Germerott, D., additional, Gizon, L., additional, Gómez Cama, J. M., additional, Guerrero, L., additional, Gutierrez-Marques, P., additional, Kolleck, M., additional, Korpi-Lagg, A., additional, Michalik, H., additional, Moreno Vacas, A., additional, Orozco Suárez, D., additional, Pérez-Grande, I., additional, Sanchis Kilders, E., additional, Balaguer Jiménez, M., additional, Schou, J., additional, Schühle, U., additional, Staub, J., additional, Strecker, H., additional, del Toro Iniesta, J. C., additional, Volkmer, R., additional, and Woch, J., additional
Published: 2023
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47. The ratio of horizontal to vertical displacement in solar oscillations estimated from combined SO/PHI and SDO/HMI observations

Author: Schou Jesper, Álvarez Herrero, Alberto, Hirzberger, J., Albert , Kinga, N. Albelo Jorge, T. Appourchaux, J. Blanco Rodríguez, Gandorfer , A., Germerott ,D., Guerrero ,L., Gutierrez-Marques ,P., Kahil ,F., Kolleck, M., Solanki ,S.K., del Toro Iniesta ,J.C., Volkmer, R., Woch , J., Fiethe , F., Pérez-Grande , I., Sanchis Kilders, E., Balaguer Jiménez, M, Bellot Rubio, L.R., Calchetti , Daniele, Carmona, M., Deutsch, W., Feller, A., Fernandez-Rico, G., Fernández-Medina, A., García Parejo, P., Gasent Blesa , J.L., Gizon , L., Grauf, B., Heerlein , K., Korpi-Lagg , A., López Jiménez, A., Maue, T., Meller, R., Moreno Vacas ,A., Müller, R., Nakai, E., Schmidt, W., Sinjan, J., Staub, J., Strecker, H, Torralbo, I., Valori, G., Schou Jesper, Álvarez Herrero, Alberto, Hirzberger, J., Albert , Kinga, N. Albelo Jorge, T. Appourchaux, J. Blanco Rodríguez, Gandorfer , A., Germerott ,D., Guerrero ,L., Gutierrez-Marques ,P., Kahil ,F., Kolleck, M., Solanki ,S.K., del Toro Iniesta ,J.C., Volkmer, R., Woch , J., Fiethe , F., Pérez-Grande , I., Sanchis Kilders, E., Balaguer Jiménez, M, Bellot Rubio, L.R., Calchetti , Daniele, Carmona, M., Deutsch, W., Feller, A., Fernandez-Rico, G., Fernández-Medina, A., García Parejo, P., Gasent Blesa , J.L., Gizon , L., Grauf, B., Heerlein , K., Korpi-Lagg , A., López Jiménez, A., Maue, T., Meller, R., Moreno Vacas ,A., Müller, R., Nakai, E., Schmidt, W., Sinjan, J., Staub, J., Strecker, H, Torralbo, I., and Valori, G.
Abstract: Received: 19 January; 2023 Accepted: 15 March 2023, In order to make accurate inferences about the solar interior using helioseismology, it is essential to understand all the relevant physical effects on the observations. One effect to understand is the (complex-valued) ratio of the horizontal to vertical displacement of the p- and f-modes at the height at which they are observed. Unfortunately, it is impossible to measure this ratio directly from a single vantage point, and it has been difficult to disentangle observationally from other effects. In this paper we attempt to measure the ratio directly using 7.5 h of simultaneous observations from the Polarimetric and Helioseismic Imager on board Solar Orbiter and the Helioseismic and Magnetic Imager on board the Solar Dynamics Observatory. While image geometry problems make it difficult to determine the exact ratio, it appears to agree well with that expected from adiabatic oscillations in a standard solar model. On the other hand it does not agree with a commonly used approximation, indicating that this approximation should not be used in helioseismic analyses. In addition, the ratio appears to be real-valued. © The Authors 2023., Agencia Española de Investigación, Federal Ministry for Economic Affairs and Energy (BMWi) (Alemania), Max Planck Gesellschaft (MPG) (Alemania), German Aerospace Center (DLR), Ministerio de Ciencia e Innovación de España, Centro Nacional de Estudios Espaciales (Francia), Depto. de Óptica, Fac. de Óptica y Optometría, TRUE, pub
Published: 2023

48. Correlation between emotion dysregulation and mood symptoms of bipolar disorder: A systematic review and meta-analysis.

Author: Oliva, V., Prisco, M. De, Fico, G., Possidente, C., Fortea, L., Montejo, L., Anmella, G., Hidalgo-Mazzei, D., Grande, I., Murru, A., Fornaro, M., Bartolomeis, A. de, Dodd, A., Fanelli, G., Fabbri, C., Serretti, A., Vieta, E., Radua, J., Oliva, V., Prisco, M. De, Fico, G., Possidente, C., Fortea, L., Montejo, L., Anmella, G., Hidalgo-Mazzei, D., Grande, I., Murru, A., Fornaro, M., Bartolomeis, A. de, Dodd, A., Fanelli, G., Fabbri, C., Serretti, A., Vieta, E., and Radua, J.
Abstract: Contains fulltext : 299975.pdf (Publisher’s version ) (Open Access), BACKGROUND: Emotion dysregulation (ED) is a transdiagnostic construct characterized by difficulties regulating intense emotions. People with bipolar disorder (BD) are more likely to show ED and use maladaptive emotion regulation strategies than adaptive ones. However, little is known about whether ED in BD is a trait or it is rather an epiphenomenon of mood symptoms. METHODS: We conducted a systematic review and meta-analysis of the evidence across major literature databases reporting correlations between measures of emotion regulation (overall ED and different emotion regulation strategies) and measures of depressive and (hypo)manic symptoms in BD from inception until April 12th, 2022. RESULTS: Fourteen studies involving 1371 individuals with BD were included in the qualitative synthesis, of which 11 reported quantitative information and were included in the meta-analysis. ED and maladaptive strategies were significantly higher during periods with more severe mood symptoms, especially depressive ones, while adaptive strategies were lower. CONCLUSION: ED significantly correlates with BD symptomatology, and it mainly occurs during mood alterations. ED may be a target for specific psychotherapeutic and pharmacological treatments, according to precision psychiatry. However, further studies are needed, including patients with mood episodes and longitudinal design, to provide more robust evidence and explore the causal direction of the associations., 01 december 2023
Published: 2023

49. Precision in bipolar disorders

Author: Grande, I., primary
Published: 2023
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50. InP-based CV-QKD PIC Transmitter

Author: Aldama, J., primary, Sarmiento, S., additional, Etcheverry, S., additional, Grande, I. López, additional, Vidarte, L. Trigo, additional, Castelvero, L., additional, Hinojosa, A., additional, Beckerwerth, T., additional, Piétri, Y., additional, Rhouni, A., additional, Diamanti, E., additional, and Pruneri, V., additional
Published: 2023
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