Zobrazeno 1 - 10
of 43
pro vyhledávání: '"Giuseppina Nigro"'
Autor:
Luca Sorriso-Valvo, Gaetano De Vita, Federico Fraternale, Alexandre Gurchumelia, Silvia Perri, Giuseppina Nigro, Filomena Catapano, Alessandro Retinò, Christopher H. K. Chen, Emiliya Yordanova, Oreste Pezzi, Khatuna Chargazia, Oleg Kharshiladze, Diana Kvaratskhelia, Christian L. Vásconez, Raffaele Marino, Olivier Le Contel, Barbara Giles, Thomas E. Moore, Roy B. Torbert, James L. Burch
Publikováno v:
Frontiers in Physics, Vol 7 (2019)
In weakly collisional space plasmas, the turbulent cascade provides most of the energy that is dissipated at small scales by various kinetic processes. Understanding the characteristics of such dissipative mechanisms requires the accurate knowledge o
Externí odkaz:
https://doaj.org/article/d83d1911c46d45a58f98165f261e3f20
Autor:
Giuseppina Nigro, Francesco Malara, Antonio Vecchio, Leonardo Primavera, Francesca Di Mare, Vincenzo Carbone, Pierluigi Veltri
Publikováno v:
Atmosphere, Vol 11, Iss 4, p 409 (2020)
Photospheric motions are believed to be the source of coronal heating and of velocity fluctuations detected in the solar corona. A numerical model, based on the shell technique applied on reduced magnetohydrodynamics equations, is used to represent e
Externí odkaz:
https://doaj.org/article/05189026f0e04cfc8c6512dec6dcbe3a
Autor:
Aaron C. Birch, Milan Maksimovic, Matts Carlsson, Malcolm Macdonald, Luis Bellot-Rubio, Giuseppina Nigro, Thierry Corbard, Patrick Boumier, Paulett C. Liewer, A. N. Fazakerley, Neil Murphy, Christopher Owen, Richard A. Harrison, Jackie A. Davies, Werner Schmutz, V. Martinez-Pillet, Takashi Sekii, John Leibacher, Louise K. Harra, D. Spadaro, Astrid Veronig, Laurent Gizon, Marco Romoli, Thierry Appourchaux, Vincenzo Andretta, Wolfgang Finsterle, Giampiero Naletto, Donald M. Hassler, Pierre Rochus, Silvano Fineschi, Robert H. Cameron, Frédéric Baudin
Publikováno v:
Experimental Astronomy
Experimental Astronomy, Springer Link, 2021, ⟨10.1007/s10686-021-09769-x⟩
Experimental Astronomy, Springer Link, 2021, ⟨10.1007/s10686-021-09769-x⟩
Full list of authors: Harra, Louise; Andretta, Vincenzo; Appourchaux, Thierry; Baudin, Frédéric; Bellot-Rubio, Luis; Birch, Aaron C.; Boumier, Patrick; Cameron, Robert H.; Carlsson, Matts; Corbard, Thierry; Davies, Jackie; Fazakerley, Andrew; Fines
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2a6a91dbd577128e3eacf6b4df46871c
http://hdl.handle.net/10261/311682
http://hdl.handle.net/10261/311682
Publikováno v:
Rendiconti lincei. Scienze fisiche e naturali 32 (2020): 25–44. doi:10.1007/s12210-020-00965-z
info:cnr-pdr/source/autori:Nigro, Giuseppina; Pegoraro, Francesco; Valentini, Francesco/titolo:Plasma physics and astrophysics: retrospects, state-of-the art, and prospects/doi:10.1007%2Fs12210-020-00965-z/rivista:Rendiconti lincei. Scienze fisiche e naturali/anno:2020/pagina_da:25/pagina_a:44/intervallo_pagine:25–44/volume:32
info:cnr-pdr/source/autori:Nigro, Giuseppina; Pegoraro, Francesco; Valentini, Francesco/titolo:Plasma physics and astrophysics: retrospects, state-of-the art, and prospects/doi:10.1007%2Fs12210-020-00965-z/rivista:Rendiconti lincei. Scienze fisiche e naturali/anno:2020/pagina_da:25/pagina_a:44/intervallo_pagine:25–44/volume:32
Within the special issue "Classical and quantum plasmas: matter under extreme conditions" a series of papers are included that were presented at the international workshop "Plasma Physics and Astrophysics up to 2020 and beyond". This meeting was held
Publikováno v:
Nonlinear Processes in Geophysics, Vol 27, Pp 175-185 (2020)
The description of the relationship between interplanetary plasma and geomagnetic activity requires complex models. Drastically reducing the ambition of describing this detailed complex interaction and, if we are interested only in the fractality pro
Autor:
Zahra Shokri, Nasibe Alipour, Hossein Safari, Pradeep Kayshap, Olena Podladchikova, Giuseppina Nigro, Durgesh Tripathi
We investigate the relationship between different transients such as blinkers detected in images taken at 304 Å, extreme ultraviolet coronal bright points (ECBPs) at 193 Å, X-ray coronal bright points (XCBPs) at 94 Å on the Atmospheric Imaging Ass
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2cf5ba19a063998249d042be18437282
Autor:
Giuseppina Nigro
Publikováno v:
Giuseppina Nigro
Low-mass M dwarf stars, T Tauri stars, as well as planets such as the Earth and Jupiter are permeated by large-scale magnetic fields generated by the convection-driven dynamo operating in their convection zones. These magnetic fields are often charac
Autor:
Leonardo Primavera, Pierluigi Veltri, Francesca Di Mare, Antonio Vecchio, Vincenzo Carbone, Francesco Malara, Giuseppina Nigro
Publikováno v:
Atmosphere, 11, 1-18
Atmosphere, Vol 11, Iss 409, p 409 (2020)
Atmosphere
Volume 11
Issue 4
Atmosphere, 11, 4, pp. 1-18
Atmosphere, Vol 11, Iss 409, p 409 (2020)
Atmosphere
Volume 11
Issue 4
Atmosphere, 11, 4, pp. 1-18
Photospheric motions are believed to be the source of coronal heating and of velocity fluctuations detected in the solar corona. A numerical model, based on the shell technique applied on reduced magnetohydrodynamics equations, is used to represent e
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a277de835baee2e3f248f8e0cabf37d7
http://hdl.handle.net/2066/220358
http://hdl.handle.net/2066/220358
The description of the relationship between interplanetary plasma and geomagnetic activity requires complex models. Drastically reducing the ambition of describing this detailed complex interaction, and if we are interested only in the fractality pro
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ff109d3c0b18a2d400fb32ae7d06038d
https://www.nonlin-processes-geophys-discuss.net/npg-2019-31/
https://www.nonlin-processes-geophys-discuss.net/npg-2019-31/
Publikováno v:
Turbulent Cascades II ISBN: 9783030125462
Spacecraft observations show the presence, in the polar Solar Wind (SW) plasma, of outward propagating Alfvenic fluctuations with a very broadband spectrum. This is true only up to a certain frequency in the spectrum, after which a consistent amount
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::cd12bd52a85aa861601414d647b06f46
https://doi.org/10.1007/978-3-030-12547-9_17
https://doi.org/10.1007/978-3-030-12547-9_17