Zobrazeno 1 - 5
of 5
pro vyhledávání: '"de Castro, G. Giménez"'
Autor:
Fernandez-Lopez, M., Benaglia, P., Cichowolski, S., Correra, F. S., Cristiani, G., Dominici, T. P., Duronea, N., de Castro, G. Gimenez, Lepine, J. R. D., Mirabel, I. F., Raulin, J. P., Saldano, H., Suad, L., Valotto, C.
The Large Latin American Millimeter Array (LLAMA for short) is a joint scientific and technological undertaking of Argentina and Brazil whose goal is to install and to operate an observing facility capable of performing observations of the Universe a
Externí odkaz:
http://arxiv.org/abs/2312.12210
Gamma-ray continuum at > 10 MeV photon energy yields information on > 0.2 - 0.3 GeV/nucleon ions at the Sun. We use the general-purpose Monte Carlo code FLUKA (FLUktuierende KAskade) to model the transport of ions injected into thick and thin target
Externí odkaz:
http://arxiv.org/abs/2009.00414
Autor:
Wedemeyer, S., Fleck, B., Battaglia, M., Labrosse, N., Fleishman, G., Hudson, H., Antolin, P., Alissandrakis, C., Ayres, T., Ballester, J., Bastian, T., Black, J., Benz, A., Brajsa, R., Carlsson, M., Costa, J., DePontieu, B., Doyle, G., de Castro, G. Gimenez, Gunár, S., Harper, G., Jafarzadeh, S., Loukitcheva, M., Nakariakov, V., Oliver, R., Schmieder, B., Selhorst, C., Shimojo, M., Simões, P., Soler, R., Temmer, M., Tiwari, S., Van Doorsselaere, T., Veronig, A., White, S., Yagoubov, P., Zaqarashvili, T.
This document was created by the Solar Simulations for the Atacama Large Millimeter Observatory Network (SSALMON) in preparation of the first regular observations of the Sun with the Atacama Large Millimeter/submillimeter Array (ALMA), which are anti
Externí odkaz:
http://arxiv.org/abs/1601.00587
Autor:
Trottet, G., Raulin, J. -P., MacKinnon, A., de Castro, G. Giménez, Simões, P. J. A., Cabezas, D., de La Luz, V., Luoni, M., Kaufmann, P.
Solar observations in the infrared domain can bring important clues on the response of the low solar atmosphere to primary energy released during flares. At present the infrared continuum has been detected at 30 THz (10 $\mu$m) in only a few flares.
Externí odkaz:
http://arxiv.org/abs/1509.06336
Autor:
Trottet, G., Raulin, J. -P., de Castro, G. Giménez, Lüthi, T., Caspi, A., Mandrini, C. H., Luoni, M. L., Kaufmann, P.
Publikováno v:
Solar Physics, Vol. 273, Issue 2, pp. 339-361; 2011 November 8
Solar flares observed in the 200-400 GHz radio domain may exhibit a slowly varying and time-extended component which follows a short (few minutes) impulsive phase and which lasts for a few tens of minutes to more than one hour. The few examples discu
Externí odkaz:
http://arxiv.org/abs/1109.5729