Zobrazeno 1 - 10
of 580
pro vyhledávání: '"Helmet streamer"'
Autor:
Serge Koutchmy, Philippe Lamy, Christian Viladrich, Boris Filippov, Arthur Nikoghossian, Leon Golub, M. Maksimovic, K. Issautier, N. Meyer-Vernet, M. Moncuquet, F. Pantellini
Publikováno v:
TWELFTH INTERNATIONAL SOLAR WIND CONFERENCE. AIP Conference Proceedings
TWELFTH INTERNATIONAL SOLAR WIND CONFERENCE. AIP Conference Proceedings, 0000, à renseigner, Unknown Region. pp.339-342, ⟨10.1063/1.3395869⟩
TWELFTH INTERNATIONAL SOLAR WIND CONFERENCE. AIP Conference Proceedings, 0000, à renseigner, Unknown Region. pp.339-342, ⟨10.1063/1.3395869⟩
International audience; Eclipse observations of the W-L corona show linear rays above active regions at times of solar maximum. We show that these linear rays are also observed in the field-of-view of the C2-LASCO coronagraph, in perfect corresponden
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bf973b1c40c395df5f19f202b04fbe23
https://hal.science/hal-03646177
https://hal.science/hal-03646177
Akademický článek
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Autor:
Benjamin J. Lynch
This report presents a three-dimensional (3D) numerical magnetohydrodynamics (MHD) model of the white-light coronagraph observational phenomena known as coronal inflows and in/out pairs. Coronal inflows in the LASCO/C2 field of view (approximately 2-
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4e87ae128a90a8d238834c1bd0c8b282
https://doi.org/10.5194/egusphere-egu21-10416
https://doi.org/10.5194/egusphere-egu21-10416
Autor:
Benoit Lavraud, Alexis P. Rouillard, Victor Réville, Chen Shi, Marco Velli, Antoine Strugarek, Anna Tenerani
Publikováno v:
The Astrophysical Journal
In contrast with the fast solar wind, that originates in coronal holes, the source of the slow solar wind is still debated. Often intermittent and enriched with low FIP elements -- akin to what is observed in closed coronal loops -- the slow wind cou
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0f263593e8f1de06b7e2c0c781aaebf3
http://arxiv.org/abs/2005.02679
http://arxiv.org/abs/2005.02679
Autor:
Jasper Halekas, N.-E. Raouafi, T. Dudok de Wit, Roberto Livi, Peter Harvey, A. Kouloumvakos, Robert J. MacDowall, Victor Réville, Benoit Lavraud, Milan Maksimovic, Michael Lavarra, Marc Pulupa, Teresa Nieves-Chinchilla, T. D. Phan, Léa Griton, Phyllis Whittlesey, Adam Szabo, Rui F. Pinto, A. P. Rouillard, N. Fargette, John W. Bonnell, Kelly E. Korreck, Nicolas Poirier, Jia Huang, R. Kieokaew, M. Berthomier, Sergio Toledo-Redondo, Anthony W. Case, Katja Klein, David M. Malaspina, Stuart D. Bale, Justin C. Kasper, Davin Larson, Philippe Louarn, Michael L. Stevens, Nicholeen M. Viall, Keith Goetz, Jonathan Eastwood, Vincent Génot
Publikováno v:
The Astrophysical journal letters
The Astrophysical journal letters, Bristol : IOP Publishing, 2020, 894 (2), pp.L19. ⟨10.3847/2041-8213/ab8d2d⟩
The Astrophysical journal letters, 2020, 894 (2), pp.L19. ⟨10.3847/2041-8213/ab8d2d⟩
The Astrophysical journal letters, Bristol : IOP Publishing, 2020, 894 (2), pp.L19. ⟨10.3847/2041-8213/ab8d2d⟩
The Astrophysical journal letters, 2020, 894 (2), pp.L19. ⟨10.3847/2041-8213/ab8d2d⟩
International audience; We present Heliospheric Current Sheet (HCS) and Plasma Sheet (HPS) observations during Parker Solar Probe's (PSP) first orbit around the Sun. We focus on the eight intervals that display a true sector boundary (TSB; based on s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::82e336d65c78322d6944335d8ca6016c
http://hdl.handle.net/20.500.12278/97882
http://hdl.handle.net/20.500.12278/97882
Publikováno v:
The Astrophysical Journal
Transverse waves are sometimes observed in solar helmet streamers, typically after the passage of a coronal mass ejection (CME). The CME-driven shock wave moves the streamer sideways, and a decaying oscillation of the streamer is observed after the C
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d4aa4206ebc9f4de7dbfdbe1ed081956
http://arxiv.org/abs/2003.12350
http://arxiv.org/abs/2003.12350
Publikováno v:
Astronomy & Astrophysics
Context. Coronal mass ejections (CMEs) on the Sun are the largest explosions in the Solar System that can drive powerful plasma shocks. The eruptions, shocks, and other processes associated to CMEs are efficient particle accelerators and the accelera
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a7e3028d1c1d9a8f8d07dfe601825177
http://hdl.handle.net/10138/320862
http://hdl.handle.net/10138/320862
Publikováno v:
The Astrophysical Journal. 916:115
Tether-cutting and Overlying Magnetic Reconnections in an MHD Simulation of Prominence-cavity System
Publikováno v:
The Astrophysical Journal. 915:55
We investigate the magnetic reconnection in an MHD simulation of a coronal magnetic flux rope (MFR) confined by a helmet streamer, where a prominence-cavity system forms. This system includes a hot cavity surrounding a prominence with prominence horn
Publikováno v:
The Astrophysical Journal
The Astrophysical Journal, American Astronomical Society, 2019
The Astrophysical Journal, 2019
The Astrophysical Journal, American Astronomical Society, 2019
The Astrophysical Journal, 2019
International audience; The release of density structures at the tip of the coronal helmet streamers, likely as a consequence of magnetic reconnection, contributes to the mass flux of the slow solar wind. In situ measurements in the vicinity of the h
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0ca8b936a8da1811f90d798cfbd6f329
https://hal.archives-ouvertes.fr/hal-02372719/file/insitupaper_20190706_revised_nomark.pdf
https://hal.archives-ouvertes.fr/hal-02372719/file/insitupaper_20190706_revised_nomark.pdf