Zobrazeno 1 - 10
of 123
pro vyhledávání: '"Umberto Villante"'
Autor:
Massimo Vellante, Andrea Piancatelli, Patrizia Francia, Marcello De Lauretis, Umberto Villante
Publikováno v:
Annals of Geophysics, Vol 52, Iss 1, Pp 27-34 (2009)
We present a statistical analysis of ULF (1-100 mHz) geomagnetic measurements conducted during years 2003-2006 at the Italian/French base of Concordia at Dome C, close to the geomagnetic pole, and at the Italian base«Mario Zucchelli» at Terra Nova
Externí odkaz:
https://doaj.org/article/68dece6a1854406fb148d1a8e4f7e1d8
Autor:
Simone Di Matteo, Larry Kepko, Nicholeen Viall, Aaron Breneman, Alexa Halford, Umberto Villante
In the solar wind density, we often observe periodic fluctuations on time scales ranging from a few minutes to a few hours which we refer to as Periodic Density Structures (PDSs). The PDSs belong to the class of “meso-scale structures” with radia
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3d48b7a470ce690c4490a7a562a0562b
https://doi.org/10.5194/egusphere-egu23-10258
https://doi.org/10.5194/egusphere-egu23-10258
Publikováno v:
Journal of Geophysical Research: Space Physics. 127
Identifying the nature and source of ultra-low frequencies (ULF) waves (
Publikováno v:
Journal of Atmospheric and Solar-Terrestrial Physics. 190:96-107
A long term analysis (1996–2015) of the occurrence and characteristics of the wave events (Pc3; f = 20–100 mHz; H and D component), detected at a low latitude ground-based station (L'Aquila, Italy), and the comparison with the ionospheric paramet
An important aspect of the interaction between the solar wind (SW) and the magnetosphere concerns the relationship between the SW structures/fluctuations and the onset/transmission of the magnetospheric wave modes. Several critical aspects may influe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d98fb4f8bbd0429a4cf36973ee96ed0c
https://doi.org/10.5194/egusphere-egu21-48
https://doi.org/10.5194/egusphere-egu21-48
Publikováno v:
Journal of Geophysical Research: Space Physics. 125
An important aspect of the interaction between the solar wind (SW) and the Earth’s magnetosphere concerns the possible relationship between SW and magnetospheric fluctuations under different SW conditions. In recent investigations (Di Matteo and Vi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6aabeecf4f6b6cee2870637782888a79
https://doi.org/10.5194/egusphere-egu2020-4516
https://doi.org/10.5194/egusphere-egu2020-4516
Autor:
Salvatore Mancuso, Ester Antonucci, L. Zangrilli, Francesco Carbone, Daniele Telloni, Roberto Bruno, Umberto Villante, Catia Grimani, Silvio Giordano
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5d7e77ea19f6f50058982c639520838b
https://hdl.handle.net/11576/2680059
https://hdl.handle.net/11576/2680059
Publikováno v:
Annals of Geophysics. 62
The International Association of Geomagnetism and Aeronomy (IAGA; one of the eight Associations of the International Union of Geodesy and Geophysics, IUGG) is concerned with the understanding and knowledge that result from studies of the magnetic and
Autor:
Umberto Villante, S. Di Matteo
Publikováno v:
Journal of Geophysical Research: Space Physics. 122:4905-4920
The occurrence of waves at discrete frequencies in the solar wind (SW) parameters has been reported in the scientific literature with some controversial results, mostly concerning the existence (and stability) of favoured sets of frequencies. On the