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2. Fan-shaped jet close to a light bridge

Author

Liu, Y., Ruan, G. P., Schmieder, B., Masson, S., Chen, Y., Su, J. T., Wang, B., Bai, X. Y., Su, Y., and Cao, Wenda

Subjects
Astrophysics - Solar and Stellar Astrophysics
Abstract

On the Sun,jets in light bridges are frequently observed with high-resolution instruments.The respective roles played by convection and the magnetic field in triggering such jets are not yet clear.We report a small fan-shaped jet along a LB observed by the 1.6m Goode Solar Telescope(GST) with the TiO Broadband Filter Imager(BFI),the Visible Imaging Spectrometer(VIS) in H{\alpha},and the Near-InfraRed Imaging Spectropolarimeter(NIRIS),along with the Stokes parameters.The high spatial and temporal resolution of those instruments allowed us to analyze the features identified during the jet event.By constructing the H{\alpha} Dopplergrams,we found that the plasma is first moving upward,whereas during the second phase of the jet,the plasma is flowing back.Working with time slice diagrams,we investigated the propagation-projected speed of the fan and its bright base.The fan-shaped jet developed within a few minutes,with diverging beams. At its base,a bright point was slipping along the LB and ultimately invaded the umbra of the sunspot.The H{\alpha} profiles of the bright points enhanced the intensity in the wings, similarly to the case of Ellerman bombs.Co-temporally,the extreme ultraviolet brightenings developed at the front of the dark material jet and moved at the same speed as the fan, leading us to propose that the fan-shaped jet material compressed and heated the ambient plasma at its extremities in the corona.Our multi-wavelength analysis indicates that the fan-shaped jet could result from magnetic reconnection across the highly diverging field low in the chromosphere,leading to an apparent slipping motion of the jet material along the LB.However,we did not find any opposite magnetic polarity at the jet base,as would typically be expected in such a configuration.We therefore discuss other plausible physical mechanisms,based on waves and convection, that may have triggered the event., Comment: 10 pages, 7 figures

Published
2022
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4. Escape of Flare-accelerated Particles in Solar Eruptive Events

Author

Masson, S., Antiochos, S. K., and DeVore, C. R.

Subjects
Astrophysics - Solar and Stellar Astrophysics, Physics - Space Physics
Abstract

Impulsive solar energetic particle events are widely believed to be due to the prompt escape into the interplanetary medium of flare-accelerated particles produced by solar eruptive events. According to the standard model for such events, however, particles accelerated by the flare reconnection should remain trapped in the flux rope comprising the coronal mass ejection. The particles should reach the Earth only much later, along with the bulk ejecta. To resolve this paradox, we have extended our previous axisymmetric model for the escape of flare-accelerated particles to fully three-dimensional (3D) geometries. We report the results of magnetohydrodynamic simulations of a coronal system that consists of a bipolar active region embedded in a background global dipole field structured by solar wind. Our simulations show that multiple magnetic reconnection episodes occur prior to and during the CME eruption and its interplanetary propagation. In addition to the episodes that build up the flux rope, reconnection between the open field and the CME couples the closed corona to the open interplanetary field. Flare-accelerated particles initially trapped in the CME thereby gain access to the open interplanetary field along a trail blazed by magnetic reconnection. A key difference between these 3D results and our previous calculations is that the interchange reconnection allows accelerated particles to escape from deep within the CME flux-rope. We estimate the spatial extent of the particle-escape channels. The relative timings between flare acceleration and release of the energetic particles through CME/open-field coupling are also determined. All our results compare favourably with observations.

Published
2019
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5. French SKA White Book - The French Community towards the Square Kilometre Array

Author

Acero, F., Acquaviva, J. -T., Adam, R., Aghanim, N., Allen, M., Alves, M., Ammanouil, R., Ansari, R., Araudo, A., Armengaud, E., Ascaso, B., Athanassoula, E., Aubert, D., Babak, S., Bacmann, A., Banday, A., Barriere, K., Bellossi, F., Bernard, J. -P., Bernardini, M. G., Béthermin, M., Blanc, E., Blanchet, L., Bobin, J., Boissier, S., Boisson, C., Boselli, A., Bosma, A., Bosse, S., Bottinelli, S., Boulanger, F., Boyer, R., Bracco, A., Briand, C., Bucher, M., Buat, V., Cambresy, L., Caillat, M., Casandjian, J. -M., Caux, E., Célestin, S., Cerruti, M., Charlot, P., Chassande-Mottin, E., Chaty, S., Christensen, N., Ciesla, L., Clerc, N., Cohen-Tanugi, J., Cognard, I., Combes, F., Comis, B., Corbel, S., Cordier, B., Coriat, M., Courtin, R., Courtois, H., Da Silva, B., Daddi, E., Dallier, R., Dartois, E., Demyk, K., Denis, J. -M., Denis, L., Djannati-Ataï, A., Donati, J. -F., Douspis, M., van Driel, W., Korso, M. N. El, Falgarone, E., Fantina, A., Farges, T., Ferrari, A., Ferrari, C., Ferrière, K., Flamary, R., Gac, N., Gauffre, S., Genova, F., Girard, J., Grenier, I., Griessmeier, J. -M., Guillard, P., Guillemot, L., Gulminelli, F., Gusdorf, A., Habart, E., Hammer, F., Hennebelle, P., Herpin, F., Hervet, O., Hughes, A., Ilbert, O., Janvier, M., Josselin, E., Julier, A., Lachaud, C., Lagache, G., Lallement, R., Lambert, S., Lamy, L., Langer, M., Larzabal, P., Lavaux, G., Bertre, T. Le, Fèvre, O. Le, Tiec, A. Le, Lefloch, B., Lehnert, M., Lemoine-Goumard, M., Levrier, F., Limousin, M., Lis, D., López-Sepulcre, A., Macias-Perez, J., Magneville, C., Marcowith, A., Margueron, J., Marquette, G., Marshall, D., Martin, L., Mary, D., Masson, S., Maurogordato, S., Mazauric, C., Mellier, Y., Miville-Deschênes, M. -A., Montier, L., Mottez, F., Mourard, D., Nesvadba, N., Nezan, J. -F., Noterdaeme, P., Novak, J., Ocvirk, P., Oertel, M., Olive, X., Ollier, V., Palanque-Delabrouille, N., Pandey-Pommier, M., Pennec, Y., Pérault, M., Peroux, C., Petit, P., Pétri, J., Petiteau, A., Pety, J., Pratt, G. W., Puech, M., Quertier, B., Raffin, E., Harison, S. Rakotozafy, Rawson, S., Renaud, M., Revenu, B., Richard, C., Richard, J., Rincon, F., Ristorcelli, I., Rodriguez, J., Schultheis, M., Schimd, C., Semelin, B., Sol, H., Starck, J. -L., Tagger, M., Tasse, C., Theureau, G., Torchinsky, S., Vastel, C., Vergani, S. D., Verstraete, L., Vigouroux, X., Vilmer, N., Vilotte, J. -P., Webb, N., Ysard, N., and Zarka, P.

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics
Abstract

The "Square Kilometre Array" (SKA) is a large international radio telescope project characterised, as suggested by its name, by a total collecting area of approximately one square kilometre, and consisting of several interferometric arrays to observe at metric and centimetric wavelengths. The deployment of the SKA will take place in two sites, in South Africa and Australia, and in two successive phases. From its Phase 1, the SKA will be one of the most formidable scientific machines ever deployed by mankind, and by far the most impressive in terms of data throughput and required computing power. With the participation of almost 200 authors from forty research institutes and six private companies, the publication of this French SKA white paper illustrates the strong involvement in the SKA project of the French astronomical community and of a rapidly growing number of major scientific and technological players in the fields of Big Data, high performance computing, energy production and storage, as well as system integration., Comment: Editor in chief: C. Ferrari; Editors: M. Alves, S. Bosse, S. Corbel, A. Ferrari, K. Ferri\`ere, S. Gauffre, E. Josselin, G. Lagache, S. Lambert, G. Marquette, J.-M. Martin, M.-A. Miville-Desch\^enes, L. Montier, B. Semelin, G. Theureau, S. Vergani, N. Vilmer, P. Zarka; Original file with high resolution figures at SKA-France link: https://ska-france.oca.eu/images/SKA-France-Media/FWB_051017.pdf

Published
2017

7. 1977-2017: 40 years of decametric observations of Jupiter and the Sun with the Nancay Decameter Array

Author

Lamy, L., Zarka, P., Cecconi, B., Klein, L. -K., Masson, S., Denis, L., Coffre, A., and Viou, C.

Subjects
Astrophysics - Solar and Stellar Astrophysics
Abstract

The Nancay Decameter Array (NDA) routinely observes low frequency (10-100 MHz) radio emissions of Jupiter and the Sun since 4 decades. The NDA observations, acquired with a variety of receivers with increasing performances, were the basis for numerous studies of jovian and solar radio emissions and now form a unique long-term database spanning >3 solar cycles and jovian revolutions. In addition, the NDA historically brought a fruitful support to space-based radio observatories of the heliosphere, to multi-wavelength analyses of solar activity and contributes to the development of space weather services. After having summarized the NDA characteristics, this article presents latest instrumental and database developments, some recent scientific results and perspectives for the next decade., Comment: Refereed article

Published
2017
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8. Flux rope, hyperbolic flux tube, and late EUV phases in a non-eruptive circular-ribbon flare

Author

Masson, S., Pariat, E., Valori, G., Deng, N., Liu, C., Wang, H., and Reid, H.

Subjects
Astrophysics - Solar and Stellar Astrophysics
Abstract

We present a detailed study of a confined circular flare dynamics associated with 3 UV late phases in order to understand more precisely which topological elements are present and how they constrain the dynamics of the flare. We perform a non-linear force free field extrapolation of the confined flare observed with the HMI and AIA instruments onboard SDO. From the 3D magnetic field we compute the squashing factor and we analyse its distribution. Conjointly, we analyse the AIA EUV light curves and images in order to identify the post-flare loops, their temporal and thermal evolution. By combining both analysis we are able to propose a detailed scenario that explains the dynamics of the flare. Our topological analysis shows that in addition to a null-point topology with the fan separatrix, the spine lines and its surrounding Quasi-Separatix Layers halo (typical for a circular flare), a flux rope and its hyperbolic flux tube (HFT) are enclosed below the null. By comparing the magnetic field topology and the EUV post-flare loops we obtain an almost perfect match 1) between the footpoints of the separatrices and the EUV 1600~\AA{} ribbons and 2) between the HFT's field line footpoints and bright spots observed inside the circular ribbons. We showed, for the first time in a confined flare, that magnetic reconnection occured initially at the HFT, below the flux rope. Reconnection at the null point between the flux rope and the overlying field is only initiated in a second phase. In addition, we showed that the EUV late phase observed after the main flare episode are caused by the cooling loops of different length which have all reconnected at the null point during the impulsive phase., Comment: Astronomy & Astrophysics, in press

Published
2017
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9. A model for stealth coronal mass ejections

Author

Lynch, B. J., Masson, S., Li, Y., DeVore, C. R., Luhmann, J. G., Antiochos, S. K., and Fisher, G. H.

Subjects
Astrophysics - Solar and Stellar Astrophysics
Abstract

Stealth coronal mass ejections (CMEs) are events in which there are almost no observable signatures of the CME eruption in the low corona but often a well-resolved slow flux rope CME observed in the coronagraph data. We present results from a three-dimensional numerical magnetohydrodynamics (MHD) simulation of the 1--2 June 2008 slow streamer blowout CME that Robbrecht et al. (2009) called "the CME from nowhere." We model the global coronal structure using a 1.4 MK isothermal solar wind and a low-order potential field source surface representation of the Carrington Rotation 2070 magnetogram synoptic map. The bipolar streamer belt arcade is energized by simple shearing flows applied in the vicinity of the helmet streamer's polarity inversion line. The flows are large scale and impart a shear typical of that expected from the differential rotation. The slow expansion of the energized helmet streamer arcade results in the formation of a radial current sheet. The subsequent onset of expansion-induced flare reconnection initiates the stealth CME while gradually releasing the stored magnetic energy. We present favorable comparisons between our simulation results and the multiviewpoint SOHO-LASCO (Large Angle and Spectrometric Coronagraph) and STEREO-SECCHI (Sun Earth Connection Coronal and Heliospheric Investigation) coronagraph observations of the preeruption streamer structure and the initiation and evolution of the stealth streamer blowout CME., Comment: 44 pages, 14 figures

Published
2016
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10. Association of high-risk coronary atherosclerosis at CCTA with clinical and circulating biomarkers: Insight from CAPIRE study

Author

Maseri, A., Andreini, D., Berti, S., Canestrari, M., Casolo, G., Gabrielli, D., Latini, R., Magnoni, M., Marraccini, P., Masson, S., Moccetti, T., Modena, M.G., Pontone, G., Gaspari, F., Ferrari, S., Cannata, A., Stucchi, N., Fois, M., Bernasconi, R., Balconi, G., Vago, T., Letizia, T., Bottazzi, B., Leone, R., Suliman, I., Sommaruga, M., Gremigni, P., Olivieri, R., Pennacchietti, L., Magnacca, M., Rossi, M.G., Pasotti, E., Clemente, A., Mushtaq, S., Mauro, E., Rossi, R., Pigazzani, F., Faggioni, L., Ciardetti, M., Puppato, M., Conte, Edoardo, Andreini, Daniele, Magnoni, Marco, Masson, Serge, Mushtaq, Saima, Berti, Sergio, Canestrari, Mauro, Casolo, Giancarlo, Gabrielli, Domenico, Latini, Roberto, Marraccini, Paolo, Moccetti, Tiziano, Modena, Maria Grazia, Pontone, Gianluca, Gorini, Marco, Maggioni, Aldo P., and Maseri, Attilio

Published
2021
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11. Formation of a rotating jet during the filament eruption on 10-11 April 2013

Author

Filippov, B., Srivastava, A. K., Dwivedi, B. N., Masson, S., Aulanier, G., Joshi, N. C., and Uddin, W.

Subjects
Astrophysics - Solar and Stellar Astrophysics
Abstract

We analyze multi-wavelength and multi-viewpoint observations of a helically twisted plasma jet formed during a confined filament eruption on 10-11 April 2013. Given a rather large scale event with its high spatial and temporal resolution observations, it allows us to clearly understand some new physical details about the formation and triggering mechanism of twisting jet. We identify a pre-existing flux rope associated with a sinistral filament, which was observed several days before the event. The confined eruption of the filament within a null point topology, also known as an Eiffel tower (or inverted-Y) magnetic field configuration results in the formation of a twisted jet after the magnetic reconnection near a null point. The sign of helicity in the jet is found to be the same as that of the sign of helicity in the filament. Untwisting motion of the reconnected magnetic field lines gives rise to the accelerating plasma along the jet axis. The event clearly shows the twist injection from the pre-eruptive magnetic field to the jet., Comment: 14 pages, 12 figures, to appear in MNRAS

Published
2015
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12. The relativistic solar particle event of 2005 January 20: origin of delayed particle acceleration

Author

Klein, K. -L., Masson, S., Bouratzis, C., Grechnev, V., Hillaris, A., and Preka-Papadema, P.

Subjects
Astrophysics - Solar and Stellar Astrophysics
Abstract

The highest energies of solar energetic nucleons detected in space or through gamma-ray emission in the solar atmosphere are in the GeV range. Where and how the particles are accelerated is still controversial. We search for observational information on the location and nature of the acceleration region(s) by comparing the timing of relativistic protons detected on Earth and radiative signatures in the solar atmosphere during the particularly well-observed 2005 Jan. 20 event. This investigation focuses on the post-impulsive flare phase, where a second peak was observed in the relativistic proton time profile by neutron monitors. This time profile is compared in detail with UV imaging and radio spectrography over a broad frequency band from the low corona to interplanetary space. It is shown that the late relativistic proton release to interplanetary space was accompanied by a distinct new episode of energy release and electron acceleration in the corona traced by the radio emission and by brightenings of UV kernels. These signatures are interpreted in terms of magnetic restructuring in the corona after the coronal mass ejection passage. We attribute the delayed relativistic proton acceleration to magnetic reconnection and possibly to turbulence in large-scale coronal loops. While Type II radio emission was observed in the high corona, no evidence of a temporal relationship with the relativistic proton acceleration was found.

Published
2014
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14. Accuracy of magnetic energy computations

Author

Valori, G., Demoulin, P., Pariat, E., and Masson, S.

Subjects
Astrophysics - Solar and Stellar Astrophysics
Abstract

For magnetically driven events, the magnetic energy of the system is the prime energy reservoir that fuels the dynamical evolution. In the solar context, the free energy is one of the main indicators used in space weather forecasts to predict the eruptivity of active regions. A trustworthy estimation of the magnetic energy is therefore needed in three-dimensional models of the solar atmosphere, eg in coronal fields reconstructions or numerical simulations. The expression of the energy of a system as the sum of its potential energy and its free energy (Thomson's theorem) is strictly valid when the magnetic field is exactly solenoidal. For numerical realizations on a discrete grid, this property may be only approximately fulfilled. We show that the imperfect solenoidality induces terms in the energy that can lead to misinterpreting the amount of free energy present in a magnetic configuration. We consider a decomposition of the energy in solenoidal and nonsolenoidal parts which allows the unambiguous estimation of the nonsolenoidal contribution to the energy. We apply this decomposition to six typical cases broadly used in solar physics. We quantify to what extent the Thomson theorem is not satisfied when approximately solenoidal fields are used. The quantified errors on energy vary from negligible to significant errors, depending on the extent of the nonsolenoidal component. We identify the main source of errors and analyze the implications of adding a variable amount of divergence to various solenoidal fields. Finally, we present pathological unphysical situations where the estimated free energy would appear to be negative, as found in some previous works, and we identify the source of this error to be the presence of a finite divergence. We provide a method of quantifying the effect of a finite divergence in numerical fields, together with detailed diagnostics of its sources.

Published
2013
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18. Interchange Slip-Running Reconnection and Sweeping SEP Beams

Author

Masson, S., Aulanier, G., Pariat, E., and Klein, K. -L.

Subjects
Astrophysics - Solar and Stellar Astrophysics
Abstract

We present a new model to explain how particles (solar energetic particles; SEPs), accelerated at a reconnection site that is not magnetically connected to the Earth, could eventually propagate along the well-connected open flux tube. Our model is based on the results of a low-beta resistive magnetohydrodynamics simulation of a three-dimensional line-tied and initially current-free bipole, that is embedded in a non-uniform open potential field. The topology of this configuration is that of an asymmetric coronal null-point, with a closed fan surface and an open outer spine. When driven by slow photospheric shearing motions, field lines, initially fully anchored below the fan dome, reconnect at the null point, and jump to the open magnetic domain. This is the standard interchange mode as sketched and calculated in 2D. The key result in 3D is that, reconnected open field lines located in the vicinity of the outer spine, keep reconnecting continuously, across an open quasi-separatrix layer, as previously identified for non-open-null-point reconnection. The apparent slipping motion of these field lines leads to form an extended narrow magnetic flux tube at high altitude. Because of the slip-running reconnection, we conjecture that if energetic particles would be traveling through, or be accelerated inside, the diffusion region, they would be successively injected along continuously reconnecting field lines that are connected farther and farther from the spine. At the scale of the full Sun, owing to the super-radial expansion of field lines below 3 solar radii, such energetic particles could easily be injected in field lines slipping over significant distances, and could eventually reach the distant flux tube that is well-connected to the Earth.

Published
2011
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19. Acceleration of Relativistic Protons during the 20 January 2005 Flare and CME

Author

Masson, S., Klein, K. -L., Buetikofer, R., Flueckiger, E., Kurt, V., Yushkov, B., and Krucker, S.

Subjects
Astrophysics - Solar and Stellar Astrophysics
Abstract

The origin of relativistic solar protons during large flare/CME events has not been uniquely identified so far.We perform a detailed comparative analysis of the time profiles of relativistic protons detected by the worldwide network of neutron monitors at Earth with electromagnetic signatures of particle acceleration in the solar corona during the large particle event of 20 January 2005. The intensity-time profile of the relativistic protons derived from the neutron monitor data indicates two successive peaks. We show that microwave, hard X-ray and gamma-ray emissions display several episodes of particle acceleration within the impulsive flare phase. The first relativistic protons detected at Earth are accelerated together with relativistic electrons and with protons that produce pion decay gamma-rays during the second episode. The second peak in the relativistic proton profile at Earth is accompanied by new signatures of particle acceleration in the corona within approximatively 1 solar radius above the photosphere, revealed by hard X-ray and microwave emissions of low intensity, and by the renewed radio emission of electron beams and of a coronal shock wave. We discuss the observations in terms of different scenarios of particle acceleration in the corona., Comment: 22 pages, 5 figures

Published
2009
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20. Anthracycline-induced cardiotoxicity: A multicenter randomised trial comparing two strategies for guiding prevention with enalapril: The International CardioOncology Society-one trial

Author

Cipolla, C.M., Cardinale, D., Ciceri, F., Latini, R., Sandri, M.T., Maggioni, A.P., Labianca, R., Tettamanti, M., Senni, M., Finzi, A., Grosso, F., Vago, T., Civelli, M., Gramenzi, S., Masson, S., Balconi, G., Bernasconi, R., Salvatici, M., Nicolis, E., Barlera, S., Magnoli, M., Buratti, M.G., Ojeda Fernandez, M.L., Franzosi, M.G., Staszewsky, L., Vasamì, A., Malossi, A., Sicuro, M., Thiebat, B., Barè, C., Corzani, A., Coccolo, F., Colecchia, S., Pellegrini, C., Bregni, M., Appio, L., Caico, I., G.Rossetti, Mesenzani, O., Campana, C., Giordano, M., Gilardoni, M., Scognamiglio, G., Corrado, G., Battagin, D., De Rosa, F., Carpino, C., Palazzo, S., Monopoli, A., Milandri, C., Giannessi, P.G., Zipoli, G., Ghisoni, F., Rizzo, A., Pastori, P., Callegari, S., Sesenna, C., Colombo, A., G.Curigliano, Fodor, C., Mangiavacchi, M., Cavina, R., Guiducci, D., Mazza, R., Turazza, F.M., Vallerio, P., Marbello, L., Sala, E., Fragasso, G., Trinca, S., Aquilina, M., Rocca, A., Farolfi, A., Andreis, D., Gori, S., Barbieri, E., Lanzoni, L., Marchetti, F., Falci, C., Bianchi, A., Mioranza, E., Banzato, A., Re, F., Gaibazzi, N., Gullo, M., Turina, M.C., Gervasi, E., Giaroli, F., Nassiacos, D., Verusio, C., Barco, B., Bertolini, A., Cucchi, G., Menatti, E., Sinagra, G., Aleksova, A., Guglielmi, A., Pinotti, G., Gueli, R., Mongiardi, C., Vallini, I., Cardinale, Daniela, Ciceri, Fabio, Latini, Roberto, Franzosi, Maria Grazia, Sandri, Maria Teresa, Civelli, Maurizio, Cucchi, GianFranco, Menatti, Elisabetta, Mangiavacchi, Maurizio, Cavina, Raffaele, Barbieri, Enrico, Gori, Stefania, Colombo, Alessandro, Curigliano, Giuseppe, Salvatici, Michela, Rizzo, Antonio, Ghisoni, Francesco, Bianchi, Alessandra, Falci, Cristina, Aquilina, Michele, Rocca, Andrea, Monopoli, Anna, Milandri, Carlo, Rossetti, Giuseppe, Bregni, Marco, Sicuro, Marco, Malossi, Alessandra, Nassiacos, Daniele, Verusio, Claudio, Giordano, Monica, Staszewsky, Lidia, Barlera, Simona, Nicolis, Enrico B., Magnoli, Michela, Masson, Serge, and Cipolla, Carlo M.

Published
2018
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26. ESICM LIVES 2016: part three: Milan, Italy. 1–5 October 2016

Author

Velasquez, T., Mackey, G., Lusk, J., Kyle, U. G., Fontenot, T., Marshall, P., Shekerdemian, L. S., Coss-Bu, J. A., Nishigaki, A., Yatabe, T., Tamura, T., Yamashita, K., Yokoyama, M., Ruiz-Rodriguez, J. C., Encina, B., Belmonte, R., Troncoso, I., Tormos, P., Riveiro, M., Baena, J., Sanchez, A., Bañeras, J., Cordón, J., Duran, N., Ruiz, A., Caballero, J., Nuvials, X., Riera, J., Serra, J., Rutten, A. M. F., van Ieperen, S. N. M., Der Kinderen, E. P. H. M., Van Logten, T., Kovacikova, L., Skrak, P., Zahorec, M., Kyle, U. G., Akcan-Arikan, A., Silva, J. C., Mackey, G., Lusk, J., Goldsworthy, M., Shekerdemian, L. S., Coss-Bu, J. A., Wood, D., Harrison, D., Parslow, R., Davis, P., Pappachan, J., Goodwin, S., Ramnarayan, P., Chernyshuk, S., Yemets, H., Zhovnir, V., Pulitano’, S. M., De Rosa, S., Mancino, A., Villa, G., Tosi, F., Franchi, P., Conti, G., Patel, B., Khine, H., Shah, A., Sung, D., Singer, L., Haghbin, S., Inaloo, S., Serati, Z., Idei, M., Nomura, T., Yamamoto, N., Sakai, Y., Yoshida, T., Matsuda, Y., Yamaguchi, Y., Takaki, S., Yamaguchi, O., Goto, T., Longani, N., Medar, S., Abdel-Aal, I. R., El Adawy, A. S., Mohammed, H. M. E. H., Mohamed, A. N., Parry, S. M., Knight, L. D., Denehy, L., De Morton, N., Baldwin, C. E., Sani, D., Kayambu, G., da Silva, V. Z. M., Phongpagdi, P., Puthucheary, Z. A., Granger, C. L., Rydingsward, J. E., Horkan, C. M., Christopher, K. B., McWilliams, D., Jones, C., Reeves, E., Atkins, G., Snelson, C., Aitken, L. M., Rattray, J., Kenardy, J., Hull, A. M., Ullman, A., Le Brocque, R., Mitchell, M., Davis, C., Macfarlane, B., Azevedo, J. C., Rocha, L. L., De Freitas, F. F. M., Cavalheiro, A. M., Lucinio, N. M., Lobato, M. S., Ebeling, G., Kraegpoeth, A., Laerkner, E., De Brito-Ashurst, I., White, C., Gregory, S., Forni, L. G., Flowers, E., Curtis, A., Wood, C. A., Siu, K., Venkatesan, K., Muhammad, J. B. H., Ng, L., Seet, E., Baptista, N., Escoval, A., Tomas, E., Agrawal, R., Mathew, R., Varma, A., Dima, E., Charitidou, E., Perivolioti, E., Pratikaki, M., Vrettou, C., Giannopoulos, A., Zakynthinos, S., Routsi, C., Atchade, E., Houzé, S., Jean-Baptiste, S., Thabut, G., Genève, C., Tanaka, S., Lortat-Jacob, B., Augustin, P., Desmard, M., Montravers, P., de Molina, F. J. González, Barbadillo, S., Alejandro, R., Álvarez-Lerma, F., Vallés, J., Catalán, R. M., Palencia, E., Jareño, A., Granada, R. M., Ignacio, M. 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Hípola, Vázquez, C. F. Lübbe, Penichet, S. M. Marrero, Campelo, F. Artiles, López, M. A. De La Cal, Santana, P. Saavedra, Santana, S. Ruíz, Repessé, X., Artiguenave, M., Paktoris-Papine, S., Espinasse, F., Dinh, A., El Sayed, F., Charron, C., Géri, G., Vieillard-Baron, A., Marmanidou, K., Oikonomou, M., Nouris, C., Dimitroulakis, K., Soilemezi, E., Matamis, D., Ferré, A., Guillot, M., Teboul, J. L., Lichtenstein, D., Mézière, G., Richard, C., Monnet, X., Pham, T., Beduneau, G., Schortgen, F., Piquilloud, L., Zogheib, E., Jonas, M., Grelon, F., Runge, I., Terzi, N., Grangé, S., Barberet, G., Guitard, P. G., Frat, J. P., Constan, A., Chrétien, J. M., Mancebo, J., Mercat, A., Richard, J. C. M., Brochard, L., Prīdāne, S., Sabeļņikovs, O., Mojoli, F., Orlando, A., Bianchi, I., Torriglia, F., Bianzina, S., Pozzi, M., Iotti, G. A., Braschi, A., Beduneau, G., Pham, T., Schortgen, F., Piquilloud, L., Zogheib, E., Jonas, M., Grelon, F., Runge, I., Terzi, N., Grangé, S., Barberet, G., Guitard, P. G., Frat, J. P., Constan, A., Chrétien, J. M., Mancebo, J., Mercat, A., Richard, J. C. M., Brochard, L., Kondili, E., Psarologakis, C., Kokkini, S., Amargianitakis, V., Babalis, D., Chytas, A., Chouvarda, I., Vaporidi, K., Georgopoulos, D., Trapp, O., Kalenka, A., Mojoli, F., Orlando, A., Bianchi, I., Torriglia, F., Bianzina, S., Pozzi, M., Iotti, G. A., Braschi, A., Lozano, J. A. Benítez, Sánchez, P. Carmona, Francioni, J. E. Barrueco, Ferrón, F. Ruiz, Simón, J. M. Serrano, Spadaro, S., Karbing, D. S., Gioia, A., Moro, F., Corte, F. Dalla, Mauri, T., Volta, C. A., Rees, S. E., Petrova, M. V., Mohan, R., Butrov, A. V., Beeharry, S. D., Vatsik, M. V., Sakieva, F. I., Gobert, F., Yonis, H., Tapponnier, R., Fernandez, R., Labaune, M. A., Burle, J. F., Barbier, J., Vincent, B., Cleyet, M., Richard, J. C., Guérin, C., Shinotsuka, C. Righy, Creteur, J., Taccone, F. S., Törnblom, S., Nisula, S., Vaara, S., Poukkanen, M., Andersson, S., Pettilä, V., Pesonen, E., Xie, Z., Liao, X., Kang, Y., Zhang, J., Kubota, K., Egi, M., Mizobuchi, S., Hegazy, S., El-Keraie, A., El Sayed, E., El Hamid, M. Abd, Rodrigues, N. J., Pereira, M., Godinho, I., Gameiro, J., Neves, M., Gouveia, J., e Silva, Z. Costa, Lopes, J. A., Mckinlay, J., Kostalas, M., Kooner, G., Dudas, G., Horton, A., Kerr, C., Karanjia, N., Creagh-Brown, B., Forni, L., Yamazaki, A., Ganuza, M. Sanz, Molina, J. A. Martinez, Martinez, F. Hidalgo, Freile, M. T. Chiquito, Fernandez, N. Garcia, Travieso, P. Medrano, Bandert, A., Frithiof, R., Lipcsey, M., Smekal, D., Schlaepfer, P., Durovray, J. D., Plouhinec, V., Chiappa, C., Bellomo, R., Schneider, A. G., Mitchell, S., Durrant, J., Street, H., Dunthorne, E., Shears, J., Caballero, C. Hernandez, Hutchison, R., Schwarze, S., Ghabina, S., Thompson, E., Prowle, J. R., Kirwan, C. J., Gonzalez, C. A., Pinto, J. L., Orozco, V., Patiño, J. A., Garcia, P. K., Contreras, K. M., Rodriguez, P., Echeverri, J. E., GETGAG Working Group, JSEPTIC (Japanese Society of Education for Physicians and Trainees in Intensive Care) Clinical Trial Group, CAPCRI Study, for the ReVA Research Network and the PROVE Network Investigators, from the FROG ICU Investigators, The WIND study group, Plug Working Group, GETGAG/SEMICYUC, AKI Research Group, St George’s University of London, IPREA Study Group, FINNRESUSCI Study Group, PICS- HCPA: Programa Intrahospitalar de Combate à Sepse do Hospital de Clínicas de Porto Alegre, ENVIN-HELICS Study Group, ARIAM registry of adult cardiac surgery, The Rapid Diagnosis of Infections in the Critically Ill Team, Tokyo Womens Medical University, PLUG working group, PLUG Working Group, On behalf of Okayama Research Investigation Organizing Network (ORION)investigators, PS-ICU Group, Japan Septic Disseminated Intravascular Coagulation (JSEPTIC DIC) study group, Student Research Committee - Shiraz University of Medical Sciences, ARIAM-ANDALUCIA, The WIND study group, PLUG Working Group, The WIND study group, PLUG Working Group, and Plug working group

Published
2016
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30. Fan-shaped jet close to a light bridge

Author

Liu, Y., primary, Ruan, G. P., additional, Schmieder, B., additional, Masson, S., additional, Chen, Y., additional, Su, J. T., additional, Wang, B., additional, Bai, X. Y., additional, Su, Y., additional, and Cao, W., additional

Published
2022
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33. EUREC4A

Author

Stevens, B, Bony, S, Farrell, D, Ament, F, Blyth, A, Fairall, C, Karstensen, J, Quinn, P, Speich, S, Acquistapace, C, Aemisegger, F, Albright, A, Bellenger, H, Bodenschatz, E, Caesar, K, Chewitt-Lucas, R, De Boer, G, Delanoe, J, Denby, L, Ewald, F, Fildier, B, Forde, M, George, G, Gross, S, Hagen, M, Hausold, A, Heywood, K, Hirsch, L, Jacob, M, Jansen, F, Kinne, S, Klocke, D, Kolling, T, Konow, H, Lothon, M, Mohr, W, Naumann, A, Nuijens, L, Olivier, L, Pincus, R, Pohlker, M, Reverdin, G, Roberts, G, Schnitt, S, Schulz, H, Pier Siebesma, A, Stephan, C, Sullivan, P, Touze-Peiffer, L, Vial, J, Vogel, R, Zuidema, P, Alexander, N, Alves, L, Arixi, S, Asmath, H, Bagheri, G, Baier, K, Bailey, A, Baranowski, D, Baron, A, Barrau, S, Barrett, P, Batier, F, Behrendt, A, Bendinger, A, Beucher, F, Bigorre, S, Blades, E, Blossey, P, Bock, O, Boing, S, Bosser, P, Bourras, D, Bouruet-Aubertot, P, Bower, K, Branellec, P, Branger, H, Brennek, M, Brewer, A, Brilouet, P, Brugmann, B, Buehler, S, Burke, E, Burton, R, Calmer, R, Canonici, J, Carton, X, Cato, G, Charles, J, Chazette, P, Chen, Y, Chilinski, M, Choularton, T, Chuang, P, Clarke, S, Coe, H, Cornet, C, Coutris, P, Couvreux, F, Crewell, S, Cronin, T, Cui, Z, Cuypers, Y, Daley, A, Damerell, G, Dauhut, T, Deneke, H, Desbios, J, Dorner, S, Donner, S, Douet, V, Drushka, K, Dutsch, M, Ehrlich, A, Emanuel, K, Emmanouilidis, A, Etienne, J, Etienne-Leblanc, S, Faure, G, Feingold, G, Ferrero, L, Fix, A, Flamant, C, Flatau, P, Foltz, G, Forster, L, Furtuna, I, Gadian, A, Galewsky, J, Gallagher, M, Gallimore, P, Gaston, C, Gentemann, C, Geyskens, N, Giez, A, Gollop, J, Gouirand, I, Gourbeyre, C, De Graaf, D, De Groot, G, Grosz, R, Guttler, J, Gutleben, M, Hall, K, Harris, G, Helfer, K, Henze, D, Herbert, C, Holanda, B, Ibanez-Landeta, A, Intrieri, J, Iyer, S, Julien, F, Kalesse, H, Kazil, J, Kellman, A, Kidane, A, Kirchner, U, Klingebiel, M, Korner, M, Kremper, L, Kretzschmar, J, Kruger, O, Kumala, W, Kurz, A, L'Hegaret, P, Labaste, M, Lachlan-Cope, T, Laing, A, Landschutzer, P, Lang, T, Lange, D, Lange, I, Laplace, C, Lavik, G, Laxenaire, R, Lebihan, C, Leandro, M, Lefevre, N, Lena, M, Lenschow, D, Li, Q, Lloyd, G, Los, S, Losi, N, Lovell, O, Luneau, C, Makuch, P, Malinowski, S, Manta, G, Marinou, E, Marsden, N, Masson, S, Maury, N, Mayer, B, Mayers-Als, M, Mazel, C, Mcgeary, W, Mcwilliams, J, Mech, M, Mehlmann, M, Meroni, A, Mieslinger, T, Minikin, A, Minnett, P, Moller, G, Avalos, Y, Muller, C, Musat, I, Napoli, A, Neuberger, A, Noisel, C, Noone, D, Nordsiek, F, Nowak, J, Oswald, L, Parker, D, Peck, C, Person, R, Philippi, M, Plueddemann, A, Pohlker, C, Portge, V, Poschl, U, Pologne, L, Posyniak, M, Prange, M, Melendez, E, Radtke, J, Ramage, K, Reimann, J, Renault, L, Reus, K, Reyes, A, Ribbe, J, Ringel, M, Ritschel, M, Rocha, C, Rochetin, N, Rottenbacher, J, Rollo, C, Royer, H, Sadoulet, P, Saffin, L, Sandiford, S, Sandu, I, Schafer, M, Schemann, V, Schirmacher, I, Schlenczek, O, Schmidt, J, Schroder, M, Schwarzenboeck, A, Sealy, A, Senff, C, Serikov, I, Shohan, S, Siddle, E, Smirnov, A, Spath, F, Spooner, B, Katharina Stolla, M, Szkolka, W, De Szoeke, S, Tarot, S, Tetoni, E, Thompson, E, Thomson, J, Tomassini, L, Totems, J, Ubele, A, Villiger, L, Von Arx, J, Wagner, T, Walther, A, Webber, B, Wendisch, M, Whitehall, S, Wiltshire, A, Wing, A, Wirth, M, Wiskandt, J, Wolf, K, Worbes, L, Wright, E, Wulfmeyer, V, Young, S, Zhang, C, Zhang, D, Ziemen, F, Zinner, T, Zoger, M, Stevens B., Bony S., Farrell D., Ament F., Blyth A., Fairall C., Karstensen J., Quinn P. K., Speich S., Acquistapace C., Aemisegger F., Albright A. L., Bellenger H., Bodenschatz E., Caesar K. -A., Chewitt-Lucas R., De Boer G., Delanoe J., Denby L., Ewald F., Fildier B., Forde M., George G., Gross S., Hagen M., Hausold A., Heywood K. J., Hirsch L., Jacob M., Jansen F., Kinne S., Klocke D., Kolling T., Konow H., Lothon M., Mohr W., Naumann A. K., Nuijens L., Olivier L., Pincus R., Pohlker M., Reverdin G., Roberts G., Schnitt S., Schulz H., Pier Siebesma A., Stephan C. C., Sullivan P., Touze-Peiffer L., Vial J., Vogel R., Zuidema P., Alexander N., Alves L., Arixi S., Asmath H., Bagheri G., Baier K., Bailey A., Baranowski D., Baron A., Barrau S., Barrett P. A., Batier F., Behrendt A., Bendinger A., Beucher F., Bigorre S., Blades E., Blossey P., Bock O., Boing S., Bosser P., Bourras D., Bouruet-Aubertot P., Bower K., Branellec P., Branger H., Brennek M., Brewer A., Brilouet P. -E., Brugmann B., Buehler S. A., Burke E., Burton R., Calmer R., Canonici J. -C., Carton X., Cato G., Charles J. A., Chazette P., Chen Y., Chilinski M. T., Choularton T., Chuang P., Clarke S., Coe H., Cornet C., Coutris P., Couvreux F., Crewell S., Cronin T., Cui Z., Cuypers Y., Daley A., Damerell G. M., Dauhut T., Deneke H., Desbios J. -P., Dorner S., Donner S., Douet V., Drushka K., Dutsch M., Ehrlich A., Emanuel K., Emmanouilidis A., Etienne J. -C., Etienne-Leblanc S., Faure G., Feingold G., Ferrero L., Fix A., Flamant C., Flatau P. J., Foltz G. R., Forster L., Furtuna I., Gadian A., Galewsky J., Gallagher M., Gallimore P., Gaston C., Gentemann C., Geyskens N., Giez A., Gollop J., Gouirand I., Gourbeyre C., De Graaf D., De Groot G. E., Grosz R., Guttler J., Gutleben M., Hall K., Harris G., Helfer K. C., Henze D., Herbert C., Holanda B., Ibanez-Landeta A., Intrieri J., Iyer S., Julien F., Kalesse H., Kazil J., Kellman A., Kidane A. T., Kirchner U., Klingebiel M., Korner M., Kremper L. A., Kretzschmar J., Kruger O., Kumala W., Kurz A., L'Hegaret P., Labaste M., Lachlan-Cope T., Laing A., Landschutzer P., Lang T., Lange D., Lange I., Laplace C., Lavik G., Laxenaire R., LeBihan C., Leandro M., Lefevre N., Lena M., Lenschow D., Li Q., Lloyd G., Los S., Losi N., Lovell O., Luneau C., Makuch P., Malinowski S., Manta G., Marinou E., Marsden N., Masson S., Maury N., Mayer B., Mayers-Als M., Mazel C., McGeary W., McWilliams J. C., Mech M., Mehlmann M., Meroni A. N., Mieslinger T., Minikin A., Minnett P., Moller G., Avalos Y. M., Muller C., Musat I., Napoli A., Neuberger A., Noisel C., Noone D., Nordsiek F., Nowak J. L., Oswald L., Parker D. J., Peck C., Person R., Philippi M., Plueddemann A., Pohlker C., Portge V., Poschl U., Pologne L., Posyniak M., Prange M., Melendez E. Q., Radtke J., Ramage K., Reimann J., Renault L., Reus K., Reyes A., Ribbe J., Ringel M., Ritschel M., Rocha C. B., Rochetin N., Rottenbacher J., Rollo C., Royer H., Sadoulet P., Saffin L., Sandiford S., Sandu I., Schafer M., Schemann V., Schirmacher I., Schlenczek O., Schmidt J., Schroder M., Schwarzenboeck A., Sealy A., Senff C. J., Serikov I., Shohan S., Siddle E., Smirnov A., Spath F., Spooner B., Katharina Stolla M., Szkolka W., De Szoeke S. P., Tarot S., Tetoni E., Thompson E., Thomson J., Tomassini L., Totems J., Ubele A. A., Villiger L., Von Arx J., Wagner T., Walther A., Webber B., Wendisch M., Whitehall S., Wiltshire A., Wing A. A., Wirth M., Wiskandt J., Wolf K., Worbes L., Wright E., Wulfmeyer V., Young S., Zhang C., Zhang D., Ziemen F., Zinner T., Zoger M., Stevens, B, Bony, S, Farrell, D, Ament, F, Blyth, A, Fairall, C, Karstensen, J, Quinn, P, Speich, S, Acquistapace, C, Aemisegger, F, Albright, A, Bellenger, H, Bodenschatz, E, Caesar, K, Chewitt-Lucas, R, De Boer, G, Delanoe, J, Denby, L, Ewald, F, Fildier, B, Forde, M, George, G, Gross, S, Hagen, M, Hausold, A, Heywood, K, Hirsch, L, Jacob, M, Jansen, F, Kinne, S, Klocke, D, Kolling, T, Konow, H, Lothon, M, Mohr, W, Naumann, A, Nuijens, L, Olivier, L, Pincus, R, Pohlker, M, Reverdin, G, Roberts, G, Schnitt, S, Schulz, H, Pier Siebesma, A, Stephan, C, Sullivan, P, Touze-Peiffer, L, Vial, J, Vogel, R, Zuidema, P, Alexander, N, Alves, L, Arixi, S, Asmath, H, Bagheri, G, Baier, K, Bailey, A, Baranowski, D, Baron, A, Barrau, S, Barrett, P, Batier, F, Behrendt, A, Bendinger, A, Beucher, F, Bigorre, S, Blades, E, Blossey, P, Bock, O, Boing, S, Bosser, P, Bourras, D, Bouruet-Aubertot, P, Bower, K, Branellec, P, Branger, H, Brennek, M, Brewer, A, Brilouet, P, Brugmann, B, Buehler, S, Burke, E, Burton, R, Calmer, R, Canonici, J, Carton, X, Cato, G, Charles, J, Chazette, P, Chen, Y, Chilinski, M, Choularton, T, Chuang, P, Clarke, S, Coe, H, Cornet, C, Coutris, P, Couvreux, F, Crewell, S, Cronin, T, Cui, Z, Cuypers, Y, Daley, A, Damerell, G, Dauhut, T, Deneke, H, Desbios, J, Dorner, S, Donner, S, Douet, V, Drushka, K, Dutsch, M, Ehrlich, A, Emanuel, K, Emmanouilidis, A, Etienne, J, Etienne-Leblanc, S, Faure, G, Feingold, G, Ferrero, L, Fix, A, Flamant, C, Flatau, P, Foltz, G, Forster, L, Furtuna, I, Gadian, A, Galewsky, J, Gallagher, M, Gallimore, P, Gaston, C, Gentemann, C, Geyskens, N, Giez, A, Gollop, J, Gouirand, I, Gourbeyre, C, De Graaf, D, De Groot, G, Grosz, R, Guttler, J, Gutleben, M, Hall, K, Harris, G, Helfer, K, Henze, D, Herbert, C, Holanda, B, Ibanez-Landeta, A, Intrieri, J, Iyer, S, Julien, F, Kalesse, H, Kazil, J, Kellman, A, Kidane, A, Kirchner, U, Klingebiel, M, Korner, M, Kremper, L, Kretzschmar, J, Kruger, O, Kumala, W, Kurz, A, L'Hegaret, P, Labaste, M, Lachlan-Cope, T, Laing, A, Landschutzer, P, Lang, T, Lange, D, Lange, I, Laplace, C, Lavik, G, Laxenaire, R, Lebihan, C, Leandro, M, Lefevre, N, Lena, M, Lenschow, D, Li, Q, Lloyd, G, Los, S, Losi, N, Lovell, O, Luneau, C, Makuch, P, Malinowski, S, Manta, G, Marinou, E, Marsden, N, Masson, S, Maury, N, Mayer, B, Mayers-Als, M, Mazel, C, Mcgeary, W, Mcwilliams, J, Mech, M, Mehlmann, M, Meroni, A, Mieslinger, T, Minikin, A, Minnett, P, Moller, G, Avalos, Y, Muller, C, Musat, I, Napoli, A, Neuberger, A, Noisel, C, Noone, D, Nordsiek, F, Nowak, J, Oswald, L, Parker, D, Peck, C, Person, R, Philippi, M, Plueddemann, A, Pohlker, C, Portge, V, Poschl, U, Pologne, L, Posyniak, M, Prange, M, Melendez, E, Radtke, J, Ramage, K, Reimann, J, Renault, L, Reus, K, Reyes, A, Ribbe, J, Ringel, M, Ritschel, M, Rocha, C, Rochetin, N, Rottenbacher, J, Rollo, C, Royer, H, Sadoulet, P, Saffin, L, Sandiford, S, Sandu, I, Schafer, M, Schemann, V, Schirmacher, I, Schlenczek, O, Schmidt, J, Schroder, M, Schwarzenboeck, A, Sealy, A, Senff, C, Serikov, I, Shohan, S, Siddle, E, Smirnov, A, Spath, F, Spooner, B, Katharina Stolla, M, Szkolka, W, De Szoeke, S, Tarot, S, Tetoni, E, Thompson, E, Thomson, J, Tomassini, L, Totems, J, Ubele, A, Villiger, L, Von Arx, J, Wagner, T, Walther, A, Webber, B, Wendisch, M, Whitehall, S, Wiltshire, A, Wing, A, Wirth, M, Wiskandt, J, Wolf, K, Worbes, L, Wright, E, Wulfmeyer, V, Young, S, Zhang, C, Zhang, D, Ziemen, F, Zinner, T, Zoger, M, Stevens B., Bony S., Farrell D., Ament F., Blyth A., Fairall C., Karstensen J., Quinn P. K., Speich S., Acquistapace C., Aemisegger F., Albright A. L., Bellenger H., Bodenschatz E., Caesar K. -A., Chewitt-Lucas R., De Boer G., Delanoe J., Denby L., Ewald F., Fildier B., Forde M., George G., Gross S., Hagen M., Hausold A., Heywood K. J., Hirsch L., Jacob M., Jansen F., Kinne S., Klocke D., Kolling T., Konow H., Lothon M., Mohr W., Naumann A. K., Nuijens L., Olivier L., Pincus R., Pohlker M., Reverdin G., Roberts G., Schnitt S., Schulz H., Pier Siebesma A., Stephan C. C., Sullivan P., Touze-Peiffer L., Vial J., Vogel R., Zuidema P., Alexander N., Alves L., Arixi S., Asmath H., Bagheri G., Baier K., Bailey A., Baranowski D., Baron A., Barrau S., Barrett P. A., Batier F., Behrendt A., Bendinger A., Beucher F., Bigorre S., Blades E., Blossey P., Bock O., Boing S., Bosser P., Bourras D., Bouruet-Aubertot P., Bower K., Branellec P., Branger H., Brennek M., Brewer A., Brilouet P. -E., Brugmann B., Buehler S. A., Burke E., Burton R., Calmer R., Canonici J. -C., Carton X., Cato G., Charles J. A., Chazette P., Chen Y., Chilinski M. T., Choularton T., Chuang P., Clarke S., Coe H., Cornet C., Coutris P., Couvreux F., Crewell S., Cronin T., Cui Z., Cuypers Y., Daley A., Damerell G. M., Dauhut T., Deneke H., Desbios J. -P., Dorner S., Donner S., Douet V., Drushka K., Dutsch M., Ehrlich A., Emanuel K., Emmanouilidis A., Etienne J. -C., Etienne-Leblanc S., Faure G., Feingold G., Ferrero L., Fix A., Flamant C., Flatau P. J., Foltz G. R., Forster L., Furtuna I., Gadian A., Galewsky J., Gallagher M., Gallimore P., Gaston C., Gentemann C., Geyskens N., Giez A., Gollop J., Gouirand I., Gourbeyre C., De Graaf D., De Groot G. E., Grosz R., Guttler J., Gutleben M., Hall K., Harris G., Helfer K. C., Henze D., Herbert C., Holanda B., Ibanez-Landeta A., Intrieri J., Iyer S., Julien F., Kalesse H., Kazil J., Kellman A., Kidane A. T., Kirchner U., Klingebiel M., Korner M., Kremper L. A., Kretzschmar J., Kruger O., Kumala W., Kurz A., L'Hegaret P., Labaste M., Lachlan-Cope T., Laing A., Landschutzer P., Lang T., Lange D., Lange I., Laplace C., Lavik G., Laxenaire R., LeBihan C., Leandro M., Lefevre N., Lena M., Lenschow D., Li Q., Lloyd G., Los S., Losi N., Lovell O., Luneau C., Makuch P., Malinowski S., Manta G., Marinou E., Marsden N., Masson S., Maury N., Mayer B., Mayers-Als M., Mazel C., McGeary W., McWilliams J. C., Mech M., Mehlmann M., Meroni A. N., Mieslinger T., Minikin A., Minnett P., Moller G., Avalos Y. M., Muller C., Musat I., Napoli A., Neuberger A., Noisel C., Noone D., Nordsiek F., Nowak J. L., Oswald L., Parker D. J., Peck C., Person R., Philippi M., Plueddemann A., Pohlker C., Portge V., Poschl U., Pologne L., Posyniak M., Prange M., Melendez E. Q., Radtke J., Ramage K., Reimann J., Renault L., Reus K., Reyes A., Ribbe J., Ringel M., Ritschel M., Rocha C. B., Rochetin N., Rottenbacher J., Rollo C., Royer H., Sadoulet P., Saffin L., Sandiford S., Sandu I., Schafer M., Schemann V., Schirmacher I., Schlenczek O., Schmidt J., Schroder M., Schwarzenboeck A., Sealy A., Senff C. J., Serikov I., Shohan S., Siddle E., Smirnov A., Spath F., Spooner B., Katharina Stolla M., Szkolka W., De Szoeke S. P., Tarot S., Tetoni E., Thompson E., Thomson J., Tomassini L., Totems J., Ubele A. A., Villiger L., Von Arx J., Wagner T., Walther A., Webber B., Wendisch M., Whitehall S., Wiltshire A., Wing A. A., Wirth M., Wiskandt J., Wolf K., Worbes L., Wright E., Wulfmeyer V., Young S., Zhang C., Zhang D., Ziemen F., Zinner T., and Zoger M.

Abstract

The science guiding the EUREC4A campaign and its measurements is presented. EUREC4A comprised roughly 5 weeks of measurements in the downstream winter trades of the North Atlantic - eastward and southeastward of Barbados. Through its ability to characterize processes operating across a wide range of scales, EUREC4A marked a turning point in our ability to observationally study factors influencing clouds in the trades, how they will respond to warming, and their link to other components of the earth system, such as upper-ocean processes or the life cycle of particulate matter. This characterization was made possible by thousands (2500) of sondes distributed to measure circulations on meso- (200 km) and larger (500 km) scales, roughly 400 h of flight time by four heavily instrumented research aircraft; four global-class research vessels; an advanced ground-based cloud observatory; scores of autonomous observing platforms operating in the upper ocean (nearly 10 000 profiles), lower atmosphere (continuous profiling), and along the air-sea interface; a network of water stable isotopologue measurements; targeted tasking of satellite remote sensing; and modeling with a new generation of weather and climate models. In addition to providing an outline of the novel measurements and their composition into a unified and coordinated campaign, the six distinct scientific facets that EUREC4A explored - from North Brazil Current rings to turbulence-induced clustering of cloud droplets and its influence on warm-rain formation - are presented along with an overview of EUREC4A's outreach activities, environmental impact, and guidelines for scientific practice. Track data for all platforms are standardized and accessible at 10.25326/165 , and a film documenting the campaign is provided as a video supplement.

Published
2021

34. Biomarkers for Traumatic Brain Injury: Data Standards and Statistical Considerations

Author

Huie, J, Mondello, S, Lindsell, C, Antiga, L, Yuh, E, Zanier, E, Masson, S, Rosario, B, Ferguson, A, Citerio, G, Huie JR, Mondello S, Lindsell CJ, Antiga L, Yuh EL, Zanier ER, Masson S, Rosario BL, Ferguson AR, Citerio G., Huie, J, Mondello, S, Lindsell, C, Antiga, L, Yuh, E, Zanier, E, Masson, S, Rosario, B, Ferguson, A, Citerio, G, Huie JR, Mondello S, Lindsell CJ, Antiga L, Yuh EL, Zanier ER, Masson S, Rosario BL, Ferguson AR, and Citerio G.

Abstract

Recent biomarker innovations hold potential for transforming diagnosis, prognostic modeling, and precision therapeutic targeting of traumatic brain injury (TBI). However, many biomarkers, including brain imaging, genomics, and proteomics, involve vast quantities of high-throughput and high-content data. Management, curation, analysis, and evidence synthesis of these data are not trivial tasks. In this review, we discuss data management concepts and statistical and data sharing strategies when dealing with biomarker data in the context of TBI research. We propose that application of biomarkers involves three distinct steps-discovery, evaluation, and evidence synthesis. First, complex/big data has to be reduced to useful data elements at the stage of biomarker discovery. Second, inferential statistical approaches must be applied to these biomarker data elements for assessment of biomarker clinical utility and validity. Last, synthesis of relevant research is required to support practice guidelines and enable health decisions informed by the highest quality, up-to-date evidence available. We focus our discussion around recent experiences from the International Traumatic Brain Injury Research (InTBIR) initiative, with a specific focus on four major clinical projects (Transforming Research and Clinical Knowledge in TBI, Collaborative European NeuroTrauma Effectiveness Research in TBI, Collaborative Research on Acute Traumatic Brain Injury in Intensive Care Medicine in Europe, and Approaches and Decisions in Acute Pediatric TBI Trial), which are currently enrolling subjects in North America and Europe. We discuss common data elements, data collection efforts, data-sharing opportunities, and challenges, as well as examine the statistical techniques required to realize successful adoption and use of biomarkers in the clinic as a foundation for precision medicine in TBI.

Published
2021

37. Power, gender, and relative income: negotiating domestic labour in female breadwinning households in the United Kingdom

Author

Masson, S, Sullivan, O, and Hamill, H

Subjects
Sociology
Abstract

In the United Kingdom, the decline of the ‘male breadwinner model’ resulting from structural changes in the economy and gender relations over the past decades has led to an increase of female breadwinning households – understood in this thesis as households where women earn more than their male partners. I present chapters examining the processes and power relations underlying the negotiation and division of domestic labour implemented in some of these households. The thesis highlights the interactions between the structural and individual levels by paying attention to the meso-level of the household and to the emotional and relational processes underlying the division of domestic labour. I present a qualitative account of these phenomena based on several types of data collected by interviewing 26 female breadwinning couples and seven individual female breadwinners. I first used a combination of two methodological tools, the Household Portrait and a time schedule inspired from time-use studies, to assess both the quantitative and qualitative division of labour in the participants’ households. I then used joint and individual face-to-face in-depth interviews to grasp both the participants’ subjectivities, and the interactions between women and men in these couples. Despite women’s relative economic power and couples’ professions of ‘gender equality’, these couples reproduced some aspects of traditional gender roles in relation to domestic labour. I argue that a ‘marital contract’ tacitly defined women’s roles as household managers and carers of the emotional sphere, leading to an unequal division of mental load and emotion work. A fundamental content of the participants’ female breadwinning marital contract was the devaluation of women’s labour. Overall, there were asymmetries of positions and power between women and men that characterised their negotiation of domestic labour. Within this context, change was restricted to specific conditions in which women’s agency was framed by their partners’ inertia.

Published
2022

43. Endothelial damage in septic shock patients as evidenced by circulating syndecan-1, sphingosine-1-phosphate and soluble VE-cadherin: a substudy of ALBIOS

Author

Piotti, A., Novelli, D., Meessen, J. M. T. A., Ferlicca, D., Coppolecchia, S., Marino, A., Salati, G., Savioli, M., Grasselli, G., Bellani, G., Pesenti, A., Masson, S., Caironi, P., Gattinoni, L., Gobbi, M., Fracasso, C., Latini, R., Bruzzone, P., Pagan, F., Russo, R., Confalonieri, A., Abbruzzese, C., Vergnano, B., Faenza, S., Siniscalchi, A., Pierucci, E., Noto, A., Pezzi, A., Spanu, P., Parrini, V., Oggioni, R., Pasetti, G. S., Casadio, M. C., Buontempo, R., Carrer, S., Piccoli, F., Rizzi, T., Caricato, A., La Sala, M., Antonaci, A., Fassini, P., Paganini, S., Porta, V., Moise, G., Marell, S., Furia, M., Urbano, M. C., Carobbi, R., Poleni, S., Kandil, H., Ballotta, A., Bettini, F., Sanseverino, M., Gatta, A., Cecchini, F., Guatteri, L., Ciceri, G., Raimondi, F., Colombo, R., Ferraris, S., Borelli, M., Bellato, V., Cancellieri, F., Senni, S., Bertocchi, E., Ferri, P., Moioli, G., Fedele, A., Molin, A., Salsi, P., Brunori, E., Elisei, D., Maggio, G., Nicola, F. G., Cavana, M., Morelli, G., Guarino, A., Isetta, M., Tulli, G., Mangani, V., Rossi, N., Ferrari, M., Bona, F., Vay, M., Bartoli, T., Gallo, M., Vettoretto, K., Morte, M. D., Boselli, E., Puscio, D., Bovo, M., Galzerano, A., Carli, M., Zagara, G., Piotti, A, Novelli, D, Meessen, J, Ferlicca, D, Coppolecchia, S, Marino, A, Salati, G, Savioli, M, Grasselli, G, Bellani, G, Pesenti, A, Masson, S, Caironi, P, Gattinoni, L, Gobbi, M, Fracasso, C, and Latini, R

Subjects
Male, Letter, medicine.medical_treatment, 030204 cardiovascular system & hematology, Critical Care and Intensive Care Medicine, Gastroenterology, 0302 clinical medicine, VE-cadherin, Sphingosine, Septic shock, 80 and over, Medicine, Endothelial dysfunction, Phosphorylation, Aged, 80 and over, lcsh:Medical emergencies. Critical care. Intensive care. First aid, Shock, Biomarker, Glycocalyx, Sphingosine-1-phosphate, Syndecan-1, Aged, Antigens, CD, Biomarkers, Cadherins, Endothelium, Female, Humans, Italy, Lysophospholipids, Middle Aged, Retrospective Studies, Shock, Septic, Extravasation, 3. Good health, CD, Endothelial stem cell, medicine.medical_specialty, Sepsis, 03 medical and health sciences, Internal medicine, Albumins, Settore MED/41 - ANESTESIOLOGIA, Renal replacement therapy, Antigens, business.industry, Septic, Research, Albumin, 030208 emergency & critical care medicine, lcsh:RC86-88.9, medicine.disease, business
Abstract

Background Septic shock is characterized by breakdown of the endothelial glycocalyx and endothelial damage, contributing to fluid extravasation, organ failure and death. Albumin has shown benefit in septic shock patients. Our aims were: (1) to identify the relations between circulating levels of syndecan-1 (SYN-1), sphingosine-1-phosphate (S1P) (endothelial glycocalyx), and VE-cadherin (endothelial cell junctions), severity of the disease, and survival; (2) to evaluate the effects of albumin supplementation on endothelial dysfunction in patients with septic shock. Methods This was a retrospective analysis of a multicenter randomized clinical trial on albumin replacement in severe sepsis or septic shock (the Albumin Italian Outcome Sepsis Trial, ALBIOS). Concentrations of SYN-1, S1P, soluble VE-cadherin and other biomarkers were measured on days 1, 2 and 7 in 375 patients with septic shock surviving up to 7 days after randomization. Results Plasma concentrations of SYN-1 and VE-cadherin rose significantly over 7 days. SYN-1 and VE-cadherin were elevated in patients with organ failure, and S1P levels were lower. SYN-1 and VE-cadherin were independently associated with renal replacement therapy requirement during ICU stay, but only SYN-1 predicted its new occurrence. Both SYN-1 and S1P, but not VE-cadherin, predicted incident coagulation failure. Only SYN-1 independently predicted 90-day mortality. Albumin significantly reduced VE-cadherin, by 9.5% (p = 0.003) at all three time points. Conclusion Circulating components of the endothelial glycocalyx and of the endothelial cell junctions provide insights into severity and progression of septic shock, with special focus on incident coagulation and renal failure. Albumin supplementation lowered circulating VE-cadherin consistently over time. Clinical Trial Registration: ALBIOS ClinicalTrials.gov number NCT00707122.

Published
2021

44. Evaluation of the hepatic bioconversion of α-linolenic acid (ALA) to eicosapentaenoic acid (EPA) and docosahexaenoic acid (DHA) in rats fed with oils from chia (Salvia hispánica) or rosa mosqueta (Rosa rubiginosa)

Author

R. Valenzuela B., J. G. Gormáz, L. Masson S., M. Vizcarra, P. Cornejo Z., A. Valenzuela B., and G. Tapia O.

Subjects
α-linolenic acid, chia oil, docosahexaenoic acid, eicosapentaenoic acid, fatty acid bioconversion, rosa mosqueta oil, Nutrition. Foods and food supply, TX341-641
Abstract

The high dietary intake of n-6 fatty acids in relation to n-3 fatty acids generates health disorders, such as cardiovascular diseases, inflammatory diseases and other chronic diseases. The consumption of fish, which is rich in n-3 fatty acids, is low in Latin America and it is necessary to seek other alternatives, such as chia oil (CO) or rosa mosqueta oil (RMO), which are rich in α-linolenic acid (ALA), the precursor of the n -3 fatty acids, eicosapentaenoic acid (EPA) and docosahexaenoic acid (DHA). This study evaluates the hepatic bioconversion of ALA to EPA and DHA and the damage to the liver (histology and transaminase) in Sprague- Dawley rats fed different vegetable oils. Four experimental groups (n = 9 animals each group) were fed the following dietary supplements for 21 days: a) sunflower oil (SFO), b) RMO, c) CO d) olive oil with fish oil added (EPA and DHA) (OO/FO). RMO and CO increased the hepatic levels of ALA, EPA and DHA and decreased the n-6/n-3 ratio compared to SFO (p < 0.05) without changes in the parameters of liver damage. It is concluded that CO and RMO may be nutritional alternatives for providing ALA for its bioconversion to EPA and DHA.

Published
2012
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46. SUPPLEMENT : VASCO–CIRENE MEASUREMENTS

Author

Vialard, J., Duvel, J. P., McPhaden, M. J., Bouruet-Aubertot, P., Ward, B., Key, E., Bourras, D., Weller, R., Minnett, P., Weill, A., Cassou, C., Eymard, L., Fristedt, T., Basdevant, C., Dandonneau, Y., Duteil, O., Izumo, T., de Boyer Montégut, C., Masson, S., Marsac, F., Menkes, C., and Kennan, S.

Published
2009

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