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154. Contribution of the European Volcanology community to the implementation of the EPOS infrastructure for accessing geoscience data

Author

Puglisi, G., Bachelery, Patricl, Geyer, Adelina, Komorowski, Jean-Christophe, Vogfjörd, Kristin, and Vougioukalakis, Georges

Subjects
Volcanology, EPOS
Abstract

The 27th IUGG General Assembly in Montréal, Québec, Canada.,vJuly 8-18, 2019., During the last decade, the European volcanological community has undertaken a process of community building in the frame of the European Plate Observing System (EPOS) projects. The tangible outcome of this effort is the `Volcano Observations¿ Thematic Core Service (VO-TCS), which aim is the definition of a clear legal and technical frame for the coordination of the European volcanology community, and management and accessibility of its huge scientific heritage. The VO-TCS is currently developing facilities allowing long-term, easy access to volcanological data and products, and interoperable services provided by its Volcano Observatories (VOs) and Research Institutions (VRIs). The VO-TCS will offer virtual access to data, products, services, and computational platforms, and it is also defining the rules and procedures to properly allow transnational access to its volcanological facilities. The portfolio of data, products, software, and services is quite broad and varied, ranging from geophysics and geochemistry to volcanology. Data collection and analysis varies from in-situ and remote sensing observations to experimental analysis and computational elaborations. Overall, the TCS VOs and VRIs will provide quantitative, high-quality observations on the European volcanoes and the geodynamic background of the surrounding areas. For the purpose, VO-TCS has been integrating the experiences gained in monitoring and studying the Italian, Icelandic, French, Spanish, Greek, and Portuguese volcanoes. A first concrete result of the implementation of the VO-TCS is the H2020 EUROVOLC project, started in February 2018, which aims at networking the European volcanological community by supporting joint research activities and virtual/physical/ remote accesses to selected facilities.

Published
2019

156. LiteBIRD: an all-sky cosmic microwave background probe of inflation

Author

Adrian, Lee, Ade, P. A. R., Akiba, Y., Alonso, D., Arnold, K., Aumont, J., Austermann, J., Baccigalupi, C., Banday, A. J., Banerji, R., Barreiro, R. B., Basak, S., Beall, J., Beckman, S., Bersanelli, M., Borrill, J., Boulanger, F., Brown, M. L., Bucher, M., Buzzelli, A., Calabrese, E., Casas, F. J., Challinor, A., Chan, V., Chinone, Y., Cliche, J. -F, Fabio Columbro, Cukierman, A., Curtis, D., Danto, P., Paolo de Bernardis, Haan, T., Marco De Petris, Dickinson, C., Dobbs, M., Dotani, T., Duband, L., Ducout, A., Duff, S., Duivenvoorden, A., Duval, J. -M, Ebisawa, K., Elleflot, T., Enokida, H., Eriksen, H. K., Errard, J., Essinger-Hileman, T., Finelli, F., Flauger, R., Franceschet, C., Fuskeland, U., Ganga, K., Gao, J. -R, Genova-Santos, R., Ghigna, T., Gomez, A., Gradziel, M. L., Grain, J., Grupp, F., Gruppuso, A., Gudmundsson, J. E., Halverson, N. W., Hargrave, P., Hasebe, T., Hasegawa, M., Hattori, M., Hazumi, M., Henrot-Versille, S., Herranz, D., Hill, C., Hilton, G., Hirota, Y., Hivon, E., Hložek, R., Hoang, D. -T, Hubmayr, J., Ichiki, K., Iida, T., Imada, H., Ishimura, K., Ishino, H., Jaehnig, G. C., Jones, M., Kaga, T., Kashima, S., Kataoka, Y., Katayama, N., Kawasaki, T., Keskitalo, R., Kibayashi, A., Kikuchi, T., Kimura, K., Kisner, T., Kobayashi, Y., Kogiso, N., Kogut, A., Kohri, K., Komatsu, E., Komatsu, K., Konishi, K., Krachmalnicoff, N., Kuo, C. L., Kurinsky, N., Kushino, A., Kuwata-Gonokami, M., Lamagna, Luca, Lattanzi, M., Lee, A. T., Linder, E., Maffei, B., Maino, D., Maki, M., Mangilli, A., Martínez-Gonzalez, E., Silvia Masi, Mathon, R., Matsumura, T., Mennella, A., Migliaccio, M., Minami, Y., Mistuda, K., Molinari, D., Montier, L., Morgante, G., Mot, B., Murata, Y., Murphy, J. A., Nagai, M., Nagata, R., Nakamura, S., Namikawa, T., Natoli, P., Nerval, S., Nishibori, T., Nishino, H., Nomura, Y., Noviello, F., O Sullivan, C., Ochi, H., Ogawa, H., Ohsaki, H., Ohta, I., Okada, N., Pagano, L., Alessandro Paiella, Paoletti, D., Patanchon, G., Francesco Piacentini, Giampaolo Pisano, Polenta, G., Poletti, D., Prouvé, T., Puglisi, G., Rambaud, D., Raum, C., Realini, S., Remazeilles, M., Roudil, G., Rubiño-Martın, J. A., Russell, M., Sakurai, H., Sakurai, Y., Sandri, M., Savini, G., Scott, D., Sekimoto, Y., Sherwin, B. D., Shinozaki, K., Shiraishi, M., Shirron, P., Signorelli, G., Smecher, G., Spizzi, P., Stever, S. L., Stompor, R., Sugai, H., Sugiyama, S., Suzuki, A., Suzuki, J., Switzer, E., Takaku, R., Takakura, H., Takakura, S., Takeda, Y., Taylor, A., Taylor, E., Terao, Y., Thompson, K. L., Thorne, B., Tomasi, M., Tomida, H., Trappe, N., Tristram, M., Tsuji, M., Tsujimoto, M., Tucker, C., Ullom, J., Uozumi, S., Utsunomiya, S., Lanen, J., Vermeulen, G., Vielva, P., Villa, F., Vissers, M., Vittorio, N., Voisin, F., Walker, I., Watanabe, N., Wehus, I., Weller, J., Westbrook, B., Winter, B., Wollack, E., Yamamoto, R., Yamasaki, N. Y., Yanagisawa, M., Yoshida, T., Yumoto, J., Zannoni, M., and Zonca, A.

Subjects
Settore FIS/02, Settore FIS/05
Published
2019

157. The Future Landscape of High-Redshift Galaxy Cluster Science

Author

Mantz, A., Allen, S.W., Battaglia, N., Benson, B., Canning, R., Ettori, S., Evrard, A., Linden, A., McDonald, M., Abidi, M., Ahmed, Z., Amin, Mustafa.A., Ansarinejad, B., Armstrong, R., Avestruz, C., Baccigalupi, C., Bandura, K., Barkhouse, W., Basu, K., Bavdhankar, C., Bender, A.N., Bernardis, P., Bischoff, C., Biviano, A., Bleem, L., Bocquet, S., Bond, J., Borgani, S., Borrill, J., Boutigny, D., Frye, B., Bruggen, M., Cai, Z., Carlstrom, J.E., Castander, F.J., Challinor, A., Clowe, D., Cohn, J.D., Comparat, J., Cooray, A., Coulton, W., Cyr-Racine, F., Daddi, E., Delabrouille, J., Dell'antonio, I., Demarteau, M., Donahue, M., Dunkley, J., Escoffier, S., Essinger-Hileman, T., Fabbian, G., Fabjan, D., Farahi, A., Foreman, S., Fraisse, A.A., Garcia, L., Gaspari, M., Gerbino, M., Gitti, M., Gluscevic, V., Gonzalez, A., Górski, K.M., Gruen, D., Gudmundsson, J.E., Gupta, N., Haan, T., Hernquist, L., Hirata, C.M., Hlozek, R., Jeltema, T., Cohen-Tanugi, J., Johnson, B., Kadota, K., Kamionkowski, M., Khatri, R., Kisner, T., Kneib, J., Knox, L., Kovetz, E.D., Krause, E., Lattanzi, M., Lau, Erwin.T., Liguori, M., Lovisari, L., Macorra, A., Masi, S., Masui, K., Maughan, B., Maurogordato, S., McMahon, J., McNamara, B., Melchior, P., Mertens, J., Meyers, J., Mirbabayi, M., More, S., Motloch, P., Moustakas, J., Mroczkowski, T., Mukherjee, S., Nagai, D., Nagy, J., Naselsky, P., Nati, F., Newburgh, L., Niemack, M.D., Nomerotski, A., Noordeh, E., Ntampaka, M., Ota, N., Page, L., Palmese, A., Penna-Lima, M., Piacentni, F., Pierpaoli, E., Plazas, A.A., Pogosian, L., Pointecouteau, E., Prakash, A., Pratt, G., Prescod-Weinstein, C., Pryke, C., Puglisi, G., Rapetti, D., Raveri, M., Reichardt, C.L., Reiprich, Thomas.H., Remazeilles, M., Rhodes, J., Ricci, M., Rocha, G., Rose, B., Rozo, E., Ruhl, J., Sadun, A., Saliwanchik, B., Schaan, E., Schmidt, R., Fromenteau, S., Sehgal, N., Senatore, L., Seo, H., Sereno, M., Shafieloo, A., Shan, H., Shandera, S., Sherwin, B.D., Simon, S., Sridhar, S., Staggs, S., Stern, D., Suzuki, A., Tsai, Y., Turriziani, S., Umilta, C., Vazza, F., Vieregg, A., Vikhlinin, A., Walker, S.A., Watson, S., Weeren, R.J. van, Weller, J., Werner, N., Whitehorn, N., Wong, K., Wright, A., Wu, W.L.K., Xu, Z., Yasini, S., Zemcov, M., Zhang, Y., Zhao, G., Zheng, Y., Zhu, N., Zhuravleva, I., Zuntz, J., Hickox, R., Churazov, E., Nulsen, P., Jones, W.C., Wang, L., and Desai, S.

Subjects
Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics::Galaxy Astrophysics
Abstract

We describe the opportunities for galaxy cluster science in the high- redshift regime where massive, virialized halos first formed and where star formation and AGN activity peaked. New observing facilities from radio to X-ray wavelengths, combining high spatial/spectral resolution with large collecting areas, are poised to uncover this population.

Published
2019

167. Complex Energy Networks Optimization for Renewables Exploitation and Efficiency Increase.

Author

Ancona, M. A., Branchini, L., De Pascale, A., Di Pietra, B., Melino, F., Puglisi, G., and Zanghirella, F.

Subjects
ELECTRIC generators, ELECTRIC heating systems, ELECTRIC power distribution grids, INDUSTRIAL costs, HEAT pumps, RENEWABLE energy sources, NATURAL gas, GENETIC algorithms
Abstract

In the next years energy grids are expected to become increasingly complex, due to the integration between traditional fossil-fueled production systems, renewable energy generators and storage technologies. In order to maximize renewables exploitation, to minimize the economic costs and to optimize the generations systems operation, a possible solution is represented by the integration of electrical grids and district heating networks. To this purpose, the energy systems typology and size optimization, as well as the networks’ optimal management, are the challenges aspects. In this context, the aim of this paper is the optimization of both the energy generation mix and the yearly operation of a complex energy network including electrical, thermal and cooling distribution. With this purpose, in this study a real district heating network currently served by a cogeneration unit and four natural gas boilers has been considered. Several scenarios have been simulated considering the addition of different energy systems – such as heat pumps, renewable generators (electrical and/or thermal) and cooling machines – and a whole year of operation has been analyzed with an in-house developed software, based on genetic algorithms and aimed at the minimization of the total cost of energy production. The results have been compared to the reference case, representing the current configuration and operation of the network, allowing to define the optimal solution, which enables to reduce the yearly operation costs of the production plant. [ABSTRACT FROM AUTHOR]

Published
2019
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173. ALMA Band 3 polarimetric follow-up of a complete sample of faint PACO sources

Author

Galluzzi, V, primary, Puglisi, G, additional, Burkutean, S, additional, Liuzzo, E, additional, Bonato, M, additional, Massardi, M, additional, Paladino, R, additional, Gregorini, L, additional, Ricci, R, additional, Trombetti, T, additional, Toffolatti, L, additional, Burigana, C, additional, Bonaldi, A, additional, Bonavera, L, additional, Casasola, V, additional, De Zotti, G, additional, Ekers, R D, additional, di Serego Alighieri, S, additional, López-Caniego, M, additional, and Tucci, M, additional

Published
2019
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177. Dynamic Deformation of ETNA Volcano Observed by GPS and SAR Interferometry

Author

Lundgren, P, Rosen, P, Webb, F, Tesauro, M, Lanari, R, Sansosi, E, Puglisi, G, Bonforte, A, and Coltelli, M

Subjects
Environment Pollution
Abstract

Synthetic aperture radar (SAR) interferometry and GPS have shown that during the quiescent period from 1993-1995 Mt. Etna volcano, Italy, inflated. Since the initiation of eruptive activity since late 1995 the deformation has been more contentious. We will explore the detailed deformation during the period from 1995-1996 spanning the late stages of inflation and the beginning of eruptive activity. We use SAR interferometry and GPS data to measure the volcano deformation. We invert the observed deformation for both simple point source. le crack elastic sources or if warranted for a spheroidal pressure So In particular, we will examine the evolution of the inflation and the transition to a lesser deflation observed at the end of 1995. We use ERS-1/2 SAR data from both ascending and descending passes to allow for dense temporal 'sampling of the deformation and to allow us to critically assess atmospheric noise. Preliminary results from interferometry suggest that the inflation rate accelerated prior to resumption of activity in 1995, while GPS data suggest a more steady inflation with some fluctuation following the start of activity. This study will compare and contrast the interferometric SAR and GPS results and will address the strengths and weaknesses of each technique towards volcano deformation studies.

Published
1999

180. Introducing distributed solar thermal power in small-scale district heating systems

Author

Zanghirella F, Canonaco J, Puglisi G, Di Pietra B, Per Kvols Heiselberg, Zanghirella, F, Canonaco, J, Puglisi, G, and Di Pietra, B

Subjects
Solar thermal, District heating, District heating, Solar thermal, Distributed generation, Distributed generation
Abstract

District Heating Systems (DHS) connected to distributed solar collectors may contribute in reaching, especially in areas with high population density, the target of 50% of the heat demand for domestic hot water, space heating and cooling provided by renewable sources, which will be mandatory in Italy, from January 1, 2017, for new and deeply renovated buildings. By means of a software platform, developed by the Energy Efficiency Department of ENEA, a small-scale district heating system located in a suburb in the Municipality of Bologna (Italy) and including residential buildings, schools, public buildings and a commercial building and heated by gas boilers was simulated. The introduction, in the simulated DHS, of one or more solar thermal fields integrated on the roofs of the buildings was studied, and sensitivity analysis on the effect of the number and the size of the solar fields on the energy and economic performance of the DHS was carried out. The energy performance of the DHS integrated with the solar fields reaches its optimum in the configuration that maximizes the local self-consumption of the produced solar energy. Using the DHS as a vector to share solar energy, the increase in the thermal losses of the DHS can be considered acceptable in the configurations with a solar production equal to or lower than the domestic heat water loads plus the heat losses of the whole DHS in summer.

Published
2016

181. 'Nose-to-brain delivery of polymeric nanoparticles'

Author

DAL MAGRO, ROBERTA, DONZELLI, ELISABETTA, BALLARINI, ELISA, SANCINI, GIULIO ALFREDO, Musumeci, T, Bonaccorso, A, Puglisi, G, DAL MAGRO, R, Musumeci, T, Bonaccorso, A, Donzelli, E, Ballarini, E, Puglisi, G, and Sancini, G

Subjects
Nanoparticle, BIO/09 - FISIOLOGIA, brain delivery, intranasal administration
Abstract

The difficulties encountered in the treatment of brain diseases with conventional pharmacological tools have created the need for innovative strategies. The combination of nanocarriers and alternative administration routes could represent an efficient approach to reach the brain. Intranasal administration (IN) provides a non-invasive option to deliver drugs to the brain, bypassing the BBB, reducing the first-pass effect and enhancing patient compliance. The objective of the present study was to investigate the biodistribution and bioavailability to the brain of polymeric nanoparticles (PNPs) after IN administration in healthy mice. PNPs were prepared with poly-lactide-co-glycolide polymer using nanoprecipitation method. PNPs had a polymodal distribution around 350 nm. The biodistribution of DiR-loaded PNPs was evaluated by means of 3D fluorescence tomography imaging. Our results show that 3h after a single IN administration, more than 5% of the injected dose was detectable in the brain. PNPs were quickly cleared from the thorax and the abdominal cavity, while the brain fluorescence slowly decreased ranging from 3.7% to 2.3% between 24h and 96h. Repeated IN administrations (2 administrations, 24h apart) provided a significant increment of PNPs-associated fluorescence in the brain, without affecting PNPs accumulation in other organs. These findings support nose-to-brain translocation of PNPs as a noninvasive strategy to enhance the bioavailability of therapeutics to the brain

Published
2016

183. A physico-chemical study on amphiphilic cyclodextrin/liposomes nanoassemblies with drug carrier potential.

Author

Musumeci, T., Bonaccorso, A., De Gaetano, F., Larsen, K. L., Pignatello, R., Mazzaglia, A., Puglisi, G., and Ventura, C. A.

Subjects
DIFFERENTIAL scanning calorimetry, MOLE fraction, MOIETIES (Chemistry), BIODEGRADABLE nanoparticles, LIPOSOMES, DRUG carriers
Abstract

In this paper, two medusa-like ACyDs, modified at the primary rim bearing four (ACyD4) and eight carbons (ACyD8) acyl chain length, and one bouquet-like CyD, modified at primary side with thiohexyl and at secondary one with oligoethylene moiety (SC6OH), were investigated for their ability to assemble in nanostructures or to form hybrid dipalmitoylphosphatidylcholine (DPPC)/ACyDs systems. The lipophilicity of these molecules and the different preparation methods used in this study (thin layer evaporation and nanoprecipitation method) significantly affect the aggregation behaviour in aqueous medium. Except for the shortest medusa-like ACyD4, the other ACyDs formed stable nanoaggregates for at least 45 days. The effect of ACyDs on the thermotropic behaviour of DPPC liposomes was also studied by differential scanning calorimetry analysis, thus elucidating their interaction with liposomes to afford hybrid liposome/ACyDs systems. The medusa-like ACyD4 cannot be used to realize nanosystems because it quickly aggregates or it induces a complete destabilization of the liposomes. At the highest concentration investigated (0.01 molar fraction), both ACyD8 and SC6OH interacted with DPPC liposomes, forming ACyD/DPPC or SC6OH/DPPC hybrid vesicular carriers. [ABSTRACT FROM AUTHOR]

Published
2020
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186. A Measurement of the Cosmic Microwave Background $B$-Mode Polarization Power Spectrum at Sub-Degree Scales from 2 years of POLARBEAR Data

Author

Polarbear, The Collaboration, Ade, P. A. R., Aguilar, M., Akiba, Y., Arnold, K., Baccigalupi, C., Barron, D., Beck, D., Bianchini, F., Boettger, D., Borrill, J., Chapman, S., Chinone, Y., Crowley, K., Cukierman, A., Dobbs, M., Ducout, A., Dünner, R., Elleflot, T., Errard, J., Fabbian, G., Feeney, S. M., Feng, C., Fujino, T., Galitzki, N., Gilbert, A., Goeckner-Wald, N., Groh, J., Hamada, T., Hall, G., Halverson, N. W., Hasegawa, M., Hazumi, M., Hill, C., Howe, L., Inoue, Y., Jaehnig, G. C., Jaffe, A. H., Jeong, O., Kaneko, D., Katayama, N., Keating, B., Keskitalo, R., Kisner, T., Krachmalnicoff, N., Kusaka, A., Le Jeune, M., Lee, A. T., Leitch, E. M., Leon, D., Linder, E., Lowry, L., Matsuda, F., Matsumura, T., Minami, Y., Montgomery, J., Navaroli, M., Nishino, H., Paar, H., Peloton, J., Pham, A. T. P., Poletti, D., Puglisi, G., Reichardt, C. L., Richards, P. L., Ross, C., Segawa, Y., Sherwin, B. D., Silva, M., Siritanasak, P., Stebor, N., Stompor, R., Suzuki, A., Tajima, O., Takakura, S., Takatori, S., Tanabe, D., Teply, G. P., Tomaru, T., Carole Tucker, Whitehorn, N., Zahn, A., AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut d'astrophysique spatiale (IAS), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS), POLARBEAR, Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Université Paris-Sud - Paris 11 (UP11)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)-Centre National d’Études Spatiales [Paris] (CNES), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), AstroParticule et Cosmologie ( APC - UMR 7164 ), Centre National de la Recherche Scientifique ( CNRS ) -Institut National de Physique Nucléaire et de Physique des Particules du CNRS ( IN2P3 ) -Observatoire de Paris-Université Paris Diderot - Paris 7 ( UPD7 ) -Commissariat à l'énergie atomique et aux énergies alternatives ( CEA ), Institut d'astrophysique spatiale ( IAS ), and Université Paris-Sud - Paris 11 ( UP11 ) -Institut national des sciences de l'Univers ( INSU - CNRS ) -Centre National de la Recherche Scientifique ( CNRS )

Subjects
large-scale structure of universe, cosmological model, Cosmology and Nongalactic Astrophysics (astro-ph.CO), satellite: Planck, [ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph], FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, dark matter: density, cosmic background radiation, gravitation: lens, cosmology: observations, cosmic background radiation: multipole, polarization: power spectrum, High Energy Physics::Experiment, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], statistical, Astrophysics - Cosmology and Nongalactic Astrophysics
Abstract

We report an improved measurement of the cosmic microwave background (CMB) $B$-mode polarization power spectrum with the POLARBEAR experiment at 150 GHz. By adding new data collected during the second season of observations (2013-2014) to re-analyzed data from the first season (2012-2013), we have reduced twofold the band-power uncertainties. The band powers are reported over angular multipoles $500 \leq \ell \leq 2100$, where the dominant $B$-mode signal is expected to be due to the gravitational lensing of $E$-modes. We reject the null hypothesis of no $B$-mode polarization at a confidence of 3.1$\sigma$ including both statistical and systematic uncertainties. We test the consistency of the measured $B$-modes with the $\Lambda$ Cold Dark Matter ($\Lambda$CDM) framework by fitting for a single lensing amplitude parameter $A_L$ relative to the Planck best-fit model prediction. We obtain $A_L = 0.60 ^{+0.26} _{-0.24} ({\rm stat}) ^{+0.00} _{-0.04}({\rm inst}) \pm 0.14 ({\rm foreground}) \pm 0.04 ({\rm multi})$, where $A_{L}=1$ is the fiducial $\Lambda$CDM value, and the details of the reported uncertainties are explained later in the manuscript., Comment: 16 pages, 10 figures. Minor changes to match the published version. For data and figures, see http://bolo.berkeley.edu/polarbear/data/polarbear_BB_2017/

Published
2017

189. Electrical characterization and tuning of the integrated POLARBEAR-2a focal plane and readout (Conference Presentation)

Author

Barron, Darcy, primary, Arnold, Kam, additional, Elleflot, Tucker, additional, Groh, John C., additional, Kaneko, Daisuke, additional, Katayama, Nobuhiko, additional, Lee, Adrian T., additional, Lowry, Lindsay N., additional, Nishino, Haruki, additional, Suzuki, Aritoki, additional, Takatori, Sayuri, additional, Ade, P., additional, Akiba, Y., additional, Ali, A., additional, Aguilar, M., additional, Anderson, A., additional, Ashton, P., additional, Avva, J., additional, Beck, D., additional, Baccigalupi, C., additional, Beckman, S., additional, Bender, A., additional, Bianchini, F., additional, Boettger, D., additional, Borrill, J., additional, Carron, J., additional, Chapman, S., additional, Chinone, Y., additional, Coppi, G., additional, Crowley, K., additional, Cukierman, A., additional, de Haan, T., additional, Dobbs, M., additional, Dunner, R., additional, Errard, J., additional, Fabbian, G., additional, Feeney, S., additional, Feng, C., additional, Fuller, G., additional, Galitzki, N., additional, Gilbert, A., additional, Goeckner-Wald, N., additional, Hamada, T., additional, Halverson, N., additional, Hasegawa, M., additional, Hazumi, M., additional, Hill, C., additional, Holzapfel, W., additional, Howe, L., additional, Inoue, Y., additional, Ito, J., additional, Jaehnig, G., additional, Jeong, O., additional, Keating, B., additional, Keskitalo, R., additional, Kisner, T., additional, Krachmalnicoff, N., additional, Kusaka, A., additional, Le Jeune, M., additional, Leon, D., additional, Linder, E., additional, Lowitz, A., additional, Madurowicz, A., additional, Mak, D., additional, Matsuda, F., additional, Matsumura, T., additional, May, A., additional, Miller, N., additional, Minami, Y., additional, Montgomery, J., additional, Natoli, T., additional, Navroli, M., additional, Peloton, J., additional, Pham, A., additional, Piccirillo, L., additional, Plambeck, D., additional, Poletti, D., additional, Puglisi, G., additional, Raum, C., additional, Rebeiz, G., additional, Reichardt, C., additional, Richards, P., additional, Roberts, H., additional, Ross, C., additional, Rotermund, K., additional, Silva Feaver, Max, additional, Segawa, Y., additional, Sherwin, B., additional, Siritanasak, P., additional, Steinmetz, L., additional, Stompor, R., additional, Tajima, O., additional, Takakura, S., additional, Tanabe, D., additional, Tat, R., additional, Teply, G., additional, Tikhomirov, A., additional, Tomaru, T., additional, Tsai, C., additional, Verges, C., additional, Westbrook, B., additional, Whitehorn, N., additional, and Zahn, A., additional

Published
2018
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194. A solar absorption cooling system for greenhouse climate control: technical evaluation

Author

SCHETTINI, Evelia, Blanco I, SCARASCIA MUGNOZZA, Giacomo, Puglisi G, Campiotti C. A, Viola C, VOX, Giuliano, Schettini, Evelia, Blanco, I, SCARASCIA MUGNOZZA, Giacomo, Puglisi, G, Campiotti C., A, Viola, C, and Vox, Giuliano

Subjects
solar cooling, greenhouse microclimate, solar cooling, energy efficiency, greenhouse microclimate, solar energy, renewable energy sources, solar energy, renewable energy sources, energy efficiency
Abstract

It is important to manage the environment inside an horticultural greenhouse in order to guarantee suitable growing condition for the crop, safety condition for the workers and energy savings. Microclimate is influenced by climatic parameters, such as solar radiation, air temperature, relative humidity, and wind speed. Evaporative systems are generally used in warm regions for commercial greenhouse cooling, however such systems require large quantity of water that is often a scarce natural resource in Mediterranean areas. Solar absorption systems can be applied for greenhouse cooling in regions with high values of solar irradiation as alternative to evaporative systems by exploiting renewable energy sources. The solar cooling system could provide significant energy-saving opportunities for cooling greenhouses in hot climates allowing the reduction of electricity and water consumption by exploiting the contemporaneity between the cooling requirements and the solar energy availability. The paper presents the technical considerations on the application of a solar absorption cooling system to a greenhouse in the Mediterranean climatic region. The aim of the research was to define the solar collector surface related to the greenhouse cultivated area and the potential of the system in terms of cooling capacity and energy consuption. The simulation study was realized based on the experimental data collected at the experimental centre of the University of Bari, Southern Italy, in order to control the air temperature of a greenhouse covered with plastic film; the greenhouse was characterized by a surface of 300 m2. The cooling system was designed by adopting suitable technologies of energy saving, in order to reduce cooling energy needs. The designed system consists of an absorption chiller having a cooling capacity of 18 kW fed by 50 m2 of evacuated-tube solar collectors coupled to a new distribution system which provides the cooling power only for the air volume surrounding the crop and not for the whole greenhouse.

Published
2014

195. Technical evaluation for a solar absorption cooling system to be applied for greenhouse climate control

Author

Blanco, I, Vox, G, Scarascia Mugnozza, G, C A, Campiotti, Viola, C, Puglisi, G, Schettini, E., Blanco, I, Vox, Giuliano, SCARASCIA MUGNOZZA, Giacomo, Campiotti C., A, Viola, C, Puglisi, G, and Schettini, Evelia

Subjects
solar cooling, greenhouse microclimate, solar energy, energy efficiency, renewable energy sources, solar energy, solar cooling, energy efficiency, greenhouse microclimate, renewable energy sources
Abstract

The management of the greenhouse environment depends on the manipulation of the climat-ic parameters, such as solar radiation, air temperature, relative humidity and carbon dioxide concentration, in order to guarantee suitable growing condition for the crop, safety condition for the workers and energy savings. Evaporative systems are generally used in warm regions for commercial greenhouse cooling, however such systems require large quantity of water that is often a scarce natural resource in Mediterranean areas. Solar absorption cooling sys-tems can be applied for greenhouse climate control in regions with high values of solar irra-diation as alternative to evaporative systems by exploiting renewable energy sources. The solar cooling system could provide significant energy-saving opportunities for cooling green-houses in hot climates allowing the reduction of electricity and water consumption by exploit-ing the contemporaneity between the cooling requirements and the solar energy availability. The paper presents the technical considerations on the application of a solar absorption cool-ing system to a Mediterranean greenhouse. The aim of the research was to define the poten-tial of the system in terms of energy absorption and the solar collector surface related to the greenhouse cultivated area. The simulation study was realized based on the experimental data collected at the experimental centre of the University of Bari, Southern Italy, in order to control the air temperature of a greenhouse covered with plastic film; the greenhouse was characterized by a surface of 300 m2. The cooling system was designed by adopting suitable technologies of energy saving, in order to reduce cooling energy needs. The designed sys-tem consists of an absorption chiller having a cooling capacity of 18 kW fed by 60 m2 of evacuated-tube solar collectors coupled to a new distribution system which provides the cooling power only for the air volume surrounding the crop and not for the whole greenhouse.

Published
2014

196. Intranasal delivery of polymeric nanoparticles in the rat: An innovative brain targeting strategy for diseases of Central Nervous System

Author

Serapide, Maria Francesca, Musumeci, T., Pellitteri, R., Bonaccorso, A., and Puglisi, G.

Subjects
inorganic chemicals, nanoparticelle, education, technology, industry, and agriculture, somministrazioni intranasali, rat, respiratory system, health care economics and organizations
Abstract

Nose to brain delivery, combining with polymeric nanocarriers (NPs), represents a promising non-invasive strategy to carry molecules into the brain, bypassing blood brain barrier. It's possible to increase the residence time against mucociliar clearance and to prolong the release in the target site, with appropriate NPs. We used spherical NPs with negative surface charge and with a mean size lower 250 nm suitable for nose to brain delivery. To detect the cellular distributions of NPs, a fluorescent neural marker, rhodamine B, was encapsulated into NPs observed on a fluorescence microscope. The aim of this study was to investigate in the rat the brain localization of the fluorescent NPs 8, 24 and 48 h after IN administration. Our data demonstrated that the NPs could be internalized into cells and their internalization was time and region dependent. In fact, within the initial 8 h, many fluorescence NPs were found around the cells. With the extension of time, the intracellular labeled NPs increased with regional differences in the brain. In fact, after 24 h the uptake of labeled NPs was prevalently found in the rostral regions, whereas after 48 h the uptake of the labeled NPs decreased in the rostral and increased in caudal regions of the brain. These findings support the hypothesis that therapeutic agents loaded NPs, utilized in this study, may have a direct access to the brain and can represent a very promising strategy for the diseases of the central nervous system.

Published
2016

197. Effect of ferulic acid-loaded nanostructured lipid carriers on tissue transglutaminase overexpression in human glioblastoma cell lines

Author

Carbone C., Campisi A., Dell'Albani P., Bonfanti R., Spatuzza M., Musumeci T., Lauro M.R., Bonaccorso A., Pignatello R., and Puglisi G.

Subjects
transglutaminase, nanostructured lipid carriers, glioblastoma, apoptosis, Ferulic acid, neoplasms, nervous system diseases
Abstract

In the U87-MG glioma cell line we assessed the effect of unloaded/NLC-loaded FA on the TG2-mediated apoptotic pathway activation, and cell cycle progression.

Published
2016

198. LiteBIRD satellite: JAXA's new strategic L-class mission for all-sky surveys of cosmic microwave background polarization

Author

Lystrup, Makenzie, Perrin, Marshall D., Hazumi, M., Ade, P.A.R., Adler, A., Allys, E., Arnold, K., Auguste, D., Aumont, J., Aurlien, R., Austermann, J., Baccigalupi, C., Banday, A. J., Banjeri, R., Barreiro, R. B., Basak, S., Beall, J., Beck, D., Beckman, S., Bermejo, J., de Bernardis, P., Bersanelli, M., Bonis, J., Borrill, J., Boulanger, F., Bounissou, S., Brilenkov, M., Brown, M., Bucher, M., Calabrese, E., Campeti, P., Carones, A., Casas, F. J., Challinor, A., Chan, V., Cheung, K., Chinone, Y., Cliche, J. F., Colombo, L., Columbro, F., Cubas, J., Cukierman, A., Curtis, D., D'Alessandro, G., Dachlythra, N., De Petris, M., Dickinson, C., Diego-Palazuelos, P., Dobbs, M., Dotani, T., Duband, L., Duff, S., Duval, J. M., Ebisawa, K., Elleflot, T., Eriksen, H. K., Errard, J., Essinger-Hileman, T., Finelli, F., Flauger, R., Franceschet, C., Fuskeland, U., Galloway, M., Ganga, K., Gao, J. R., Genova-Santos, R., Gerbino, M., Gervasi, M., Ghigna, T., Gjerløw, E., Gradziel, M. L., Grain, J., Grupp, F., Gruppuso, A., Gudmundsson, J. E., de Haan, T., Halverson, N. W., Hargrave, P., Hasebe, T., Hasegawa, M., Hattori, M., Henrot-Versillé, S., Herman, D., Herranz, D., Hill, C. A., Hilton, G., Hirota, Y., Hivon, E., Hlozek, R. A., Hoshino, Y., de la Hoz, E., Hubmayr, J., Ichiki, K., Iida, T., Imada, H., Ishimura, K., Ishino, H., Jaehnig, G., Kaga, T., Kashima, S., Katayama, N., Kato, A., Kawasaki, T., Keskitalo, R., Kisner, T., Kobayashi, Y., Kogiso, N., Kogut, A., Kohri, K., Komatsu, E., Komatsu, K., Konishi, K., Krachmalnicoff, N., Kreykenbohm, I., Kuo, C. L., Kushino, A., Lamagna, L., Lanen, J. V., Lattanzi, M., Lee, A. T., Leloup, C., Levrier, F., Linder, E., Louis, T., Luzzi, G., Maciaszek, T., Maffei, B., Maino, D., Maki, M., Mandelli, S., Martinez-Gonzalez, E., Masi, S., Matsumura, T., Mennella, A., Migliaccio, M., Minami, Y., Mitsuda, K., Montgomery, J., Montier, L., Morgante, G., Mot, B., Murata, Y., Murphy, J. A., Nagai, M., Nagano, Y., Nagasaki, T., Nagata, R., Nakamura, S., Namikawa, T., Natoli, P., Nerval, S., Nishibori, T., Nishino, H., Noviello, F., O'Sullivan, C., Ogawa, H., Ogawa, H., Oguri, S., Ohsaki, H., Ohta, I. S., Okada, N., Okada, N., Pagano, L., Paiella, A., Paoletti, D., Patanchon, G., Peloton, J., Piacentini, F., Pisano, G., Polenta, G., Poletti, D., Prouvé, T., Puglisi, G., Rambaud, D., Raum, C., Realini, S., Reinecke, M., Remazeilles, M., Ritacco, A., Roudil, G., Rubino-Martin, J. A., Russell, M., Sakurai, H., Sakurai, Y., Sandri, M., Sasaki, M., Savini, G., Scott, D., Seibert, J., Sekimoto, Y., Sherwin, B., Shinozaki, K., Shiraishi, M., Shirron, P., Signorelli, G., Smecher, G., Stever, S., Stompor, R., Sugai, H., Sugiyama, S., Suzuki, A., Suzuki, J., Svalheim, T. L., Switzer, E., Takaku, R., Takakura, H., Takakura, S., Takase, Y., Takeda, Y., Tartari, A., Taylor, E., Terao, Y., Thommesen, H., Thompson, K. L., Thorne, B., Toda, T., Tomasi, M., Tominaga, M., Trappe, N., Tristram, M., Tsuji, M., Tsujimoto, M., Tucker, C., Ullom, J., Vermeulen, G., Vielva, P., Villa, F., Vissers, M., Vittorio, N., Wehus, I., Weller, J., Westbrook, B., Wilms, J., Winter, B., Wollack, E. J., Yamasaki, N. Y., Yoshida, T., Yumoto, J., Zannoni, M., and Zonca, A.

Published
2020
Full Text
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199. Overview of the medium and high frequency telescopes of the LiteBIRD space mission

Author

Lystrup, Makenzie, Perrin, Marshall D., Montier, L., Mot, B., de Bernardis, P., Maffei, B., Pisano, G., Columbro, F., Gudmundsson, J. E., Henrot-Versillé, S., Lamagna, L., Montgomery, J., Prouvé, T., Russell, M., Savini, G., Stever, S., Thompson, K. L., Tsujimoto, M., Tucker, C., Westbrook, B., Ade, P. A. R., Adler, A., Allys, E., Arnold, K., Auguste, D., Aumont, J., Aurlien, R., Austermann, J., Baccigalupi, C., Banday, A. J., Banerji, R., Barreiro, R. B., Basak, S., Beall, J., Beck, D., Beckman, S., Bermejo, J., Bersanelli, M., Bonis, J., Borrill, J., Boulanger, F., Bounissou, S., Brilenkov, M., Brown, M., Bucher, M., Calabrese, E., Campeti, P., Carones, A., Casas, F. J., Challinor, A., Chan, V., Cheung, K., Chinone, Y., Cliche, J. F., Colombo, L., Cubas, J., Cukierman, A., Curtis, D., D'Alessandro, G., Dachlythra, N., De Petris, M., Dickinson, C., Diego-Palazuelos, P., Dobbs, M., Dotani, T., Duband, L., Duff, S., Duval, J. M., Ebisawa, K., Elleflot, T., Eriksen, H. K., Errard, J., Essinger-Hileman, T., Finelli, F., Flauger, R., Franceschet, C., Fuskeland, U., Galloway, M., Ganga, K., Gao, J. R., Genova-Santos, R., Gerbino, M., Gervasi, M., Ghigna, T., Gjerløw, E., Gradziel, M. L., Grain, J., Grupp, F., Gruppuso, A., de Haan, T., Halverson, N. W., Hargrave, P., Hasebe, T., Hasegawa, M., Hattori, M., Hazumi, M., Herman, D., Herranz, D., Hill, C. A., Hilton, G., Hirota, Y., Hivon, E., Hlozek, R. A., Hoshino, Y., de la Hoz, E., Hubmayr, J., Ichiki, K., Iida, T., Imada, H., Ishimura, K., Ishino, H., Jaehnig, G., Kaga, T., Kashima, S., Katayama, N., Kato, A., Kawasaki, T., Keskitalo, R., Kisner, T., Kobayashi, Y., Kogiso, N., Kogut, A., Kohri, K., Komatsu, E., Komatsu, K., Konishi, K., Krachmalnicoff, N., Kreykenbohm, I., Kuo, C. L., Kushino, A., Lanen, J. V., Lattanzi, M., Lee, A. T., Leloup, C., Levrier, F., Linder, E., Louis, T., Luzzi, G., Maciaszek, T., Maino, D., Maki, M., Mandelli, S., Martinez-Gonzalez, E., Masi, S., Matsumura, T., Mennella, A., Migliaccio, M., Minami, Y., Mitsuda, K., Morgante, G., Murata, Y., Murphy, J. A., Nagai, M., Nagano, Y., Nagasaki, T., Nagata, R., Nakamura, S., Namikawa, T., Natoli, P., Nerval, S., Nishibori, T., Nishino, H., O'Sullivan, C., Ogawa, H., Ogawa, H., Oguri, S., Ohsaki, H., Ohta, I. S., Okada, N., Okada, N., Pagano, L., Paiella, A., Paoletti, D., Patanchon, G., Peloton, J., Piacentini, F., Polenta, G., Poletti, D., Puglisi, G., Rambaud, D., Raum, C., Realini, S., Reinecke, M., Remazeilles, M., Ritacco, A., Roudil, G., Rubino-Martin, J. A., Sakurai, H., Sakurai, Y., Sandri, M., Sasaki, M., Scott, D., Seibert, J., Sekimoto, Y., Sherwin, B., Shinozaki, K., Shiraishi, M., Shirron, P., Signorelli, G., Smecher, G., Stompor, R., Sugai, H., Sugiyama, S., Suzuki, A., Suzuki, J., Svalheim, T. L., Switzer, E., Takaku, R., Takakura, H., Takakura, S., Takase, Y., Takeda, Y., Tartari, A., Taylor, E., Terao, Y., Thommesen, H., Thorne, B., Toda, T., Tomasi, M., Tominaga, M., Trappe, N., Tristram, M., Tsuji, M., Ullom, J., Vermeulen, G., Vielva, P., Villa, F., Vissers, M., Vittorio, N., Wehus, I., Weller, J., Wilms, J., Winter, B., Wollack, E. J., Yamasaki, N. Y., Yoshida, T., Yumoto, J., Zannoni, M., and Zonca, A.

Published
2020
Full Text
View/download PDF

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