Zobrazeno 1 - 10
of 3 913
pro vyhledávání: '"GIORDANO S."'
Autor:
Russano, G., Andretta, V., De Leo, Y., Teriaca, L., Uslenghi, M., Giordano, S., Telloni, D., Heinzel, P., č, S. Jej či, Abbo, L., Bemporad, A., Burtovoi, A., Capuano, G. E., Frassati, F., Guglielmino, S., Jerse, G., Landini, F., Liberatore, A., Nicolini, G., Pancrazzi, M., Romano, P., Sasso, C., Susino, R., Zangrilli, L., Da Deppo, V., Fineschi, S., Grimani, C., Moses, J. D., Naletto, G., Romoli, M., Spadaro, D., Stangalini, M.
Metis, the coronagraph on board Solar Orbiter, provides for the first time coronagraphic imaging in the ultraviolet HI Ly-alpha line and, simultaneously, in polarized visible light, thus providing a host of information on the properties of CMEs and s
Externí odkaz:
http://arxiv.org/abs/2312.01899
Autor:
Demuytere J, Carlier C, Van de Sande L, Hoorens A, De Clercq K, Giordano S, Morosi L, Matteo C, Zucchetti M, Davoli E, Van Dorpe J, Vervaet C, Ceelen W
Publikováno v:
International Journal of Nanomedicine, Vol Volume 19, Pp 429-440 (2024)
Jesse Demuytere,1,* Charlotte Carlier,1,* Leen Van de Sande,1 Anne Hoorens,2 Kaat De Clercq,3 Silvia Giordano,4 Lavinia Morosi,4 Cristina Matteo,4 Massimo Zucchetti,4 Enrico Davoli,4 Jo Van Dorpe,2 Chris Vervaet,3 Wim Ceelen1 1Department of G
Externí odkaz:
https://doaj.org/article/4de5e3016ae64aa2930cccc535c710b0
Ultraviolet spectra of Comet 96/P Machholz were obtained during its 2002 perihelion with the UVCS instrument aboard the SOHO satellite. Emission from H I, C II, C III, and O I, is detected near the nucleus. The outgassing rate is in line with the val
Externí odkaz:
http://arxiv.org/abs/2111.15644
This work deals with the analysis of longitudinal ordinal responses. The novelty of the proposed approach is in modeling simultaneously the temporal dynamics of a latent trait of interest, measured via the observed ordinal responses, and the answerin
Externí odkaz:
http://arxiv.org/abs/2111.13370
Autor:
Capuano, G. E., Dolei, S., Spadaro, D., Guglielmino, S. L., Romano, P., Ventura, R., Andretta, V., Bemporad, A., Sasso, C., Susino, R., Da Deppo, V., Frassetto, F., Giordano, S. M., Landini, F., Nicolini, G., Pancrazzi, M., Romoli, M., Zangrilli, L.
Publikováno v:
A&A 652, A85 (2021)
The determination of solar wind outflow velocity is fundamental in order to probe the mechanisms of wind acceleration in the corona. We aim to study, via the Doppler dimming technique, the effects that the chromospheric Ly{\alpha} line profile shape
Externí odkaz:
http://arxiv.org/abs/2108.05957
Autor:
Mancuso, S., Bemporad, A., Frassati, F., Barghini, D., Giordano, S., Telloni, D., Taricco, C.
Publikováno v:
A&A 651, L14 (2021)
We report the first unambiguous observational evidence in the radio range of the reflection of a coronal shock wave at the boundary of a coronal hole. The event occurred above an active region located at the northwest limb of the Sun and was characte
Externí odkaz:
http://arxiv.org/abs/2107.05931
Autor:
Romoli, M., Antonucci, E., Andretta, V., Capuano, G. E., Da Deppo, V., De Leo, Y., Downs, C., Fineschi, S., Heinzel, P., Landini, F., Liberatore, A., Naletto, G., Nicolini, G., Pancrazzi, M., Sasso, C., Spadaro, D., Susino, R., Telloni, D., Teriaca, L., Uslenghi, M., Wang, Y. M., Bemporad, A., Capobianco, G., Casti, M., Fabi, M., Frassati, F., Frassetto, F., Giordano, S., Grimani, C., Jerse, G., Magli, E., Massone, G., Messerotti, M., Moses, D., Pelizzo, M. G., Romano, P., Schühle, U., Slemer, A., Stangalini, M., Straus, T., Volpicelli, C. A., Zangrilli, L., Zuppella, P., Abbo, L., Auchére, F., Cuadrado, R. Aznar, Berlicki, A., Bruno, R., Ciaravella, A., D'Amicis, R., Lamy, P., Lanzafame, A., Malvezzi, A. M., Nicolosi, P., Nisticò, G., Peter, H., Plainaki, C., Poletto, L., Reale, F., Solanki, S. K., Strachan, L., Tondello, G., Tsinganos, K., Velli, M., Ventura, R., Vial, J. C., Woch, J., Zimbardo, G.
Publikováno v:
A&A, 2021, Forthcoming article
The investigation of the wind in the solar corona initiated with the observations of the resonantly scattered UV emission of the coronal plasma obtained with UVCS-SOHO, designed to measure the wind outflow speed by applying the Doppler dimming diagno
Externí odkaz:
http://arxiv.org/abs/2106.13344
Autor:
Bemporad, A., Abbo, L., Barghini, D., Benna, C., Biondo, R., Bonino, D., Capobianco, G., Carella, F., Cora, A., Fineschi, S., Frassati, F., Gardiol, D., Giordano, S., Liberatore, A., Mancuso, S., Mignone, A., Rasetti, S., Reale, F., Riva, A., Salvati, F., Susino, R., Volpicelli, A., Zangrilli, L.
Publikováno v:
Published in the INAF Technical Reports series, num. 40, 2020 (https://openaccess.inaf.it/handle/20.500.12386/27715)
SWELTO -- Space WEather Laboratory in Turin Observatory is a conceptual framework where new ideas for the analysis of space-based and ground-based data are developed and tested. The input data are (but not limited to) remote sensing observations (EUV
Externí odkaz:
http://arxiv.org/abs/2101.07037
Publikováno v:
A&A 644, A18 (2020)
For the purpose of investigating the differential rotation of the solar corona, we analyzed ultraviolet (UV) spectral line observations acquired on both the east and west limbs at 1.7 $R_{\odot}$ by SOHO/UVCS during the solar minimum preceding solar
Externí odkaz:
http://arxiv.org/abs/2010.06353
Autor:
Zangrilli, L., Giordano, S. M.
Context. Several physical properties of solar polar plumes have been identified by different published studies, however such studies are rare and sometimes in disagreement. Aims. The purpose of the present work is to analyze a set of SOHO/UVCS data d
Externí odkaz:
http://arxiv.org/abs/2009.00627