Zobrazeno 1 - 10
of 295
pro vyhledávání: '"N. Meyer Vernet"'
Autor:
S. Kočiščák, A. Kvammen, I. Mann, N. Meyer-Vernet, D. Píša, J. Souček, A. Theodorsen, J. Vaverka, A. Zaslavsky
Publikováno v:
Annales Geophysicae, Vol 42, Pp 191-212 (2024)
Solar Orbiter is equipped with electrical antennas performing fast measurements of the surrounding electric field. The antennas register high-velocity dust impacts through the electrical signatures of impact ionization. Although the basic principle o
Externí odkaz:
https://doaj.org/article/feb594129b644bf5a214a7e48cc89581
Autor:
I. Mann, L. Nouzák, J. Vaverka, T. Antonsen, Å. Fredriksen, K. Issautier, D. Malaspina, N. Meyer-Vernet, J. Pavlů, Z. Sternovsky, J. Stude, S. Ye, A. Zaslavsky
Publikováno v:
Annales Geophysicae, Vol 37, Pp 1121-1140 (2019)
The electric and magnetic field instrument suite FIELDS on board the NASA Parker Solar Probe and the radio and plasma waves instrument RPW on the ESA Solar Orbiter mission that explore the inner heliosphere are sensitive to signals generated by dust
Externí odkaz:
https://doaj.org/article/bcdc1f30d7f94946a292b686efb73190
Autor:
M. Liu, K. Issautier, M. Moncuquet, N. Meyer-Vernet, M. Maksimovic, J. Huang, M. M. Martinovic, L. Griton, N. Chrysaphi, V. K. Jagarlamudi, S. D. Bale, M. Pulupa, J. C. Kasper, M. L. Stevens
Publikováno v:
Astronomy & Astrophysics. 674:A49
The Quasi-thermal noise (QTN) technique is a reliable tool to yield accurate measurements of the electron parameters in the solar wind. We apply this method on Parker Solar Probe (PSP) observations to derive the total electron temperature ($T_e$) fro
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::77a78890e4eb3c62a728121f4a256a4e
https://doi.org/10.1051/0004-6361/202245450
https://doi.org/10.1051/0004-6361/202245450
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
Context. Dust impacts have been observed using radio and wave instruments onboard spacecraft since the 1980s. Voltage waveforms show typical impulsive signals generated by dust grains. Aims. We aim at developing models of how signals are generated to
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::78379758cb29448e62688135362e6831
https://doi.org/10.5194/egusphere-egu22-4363
https://doi.org/10.5194/egusphere-egu22-4363
A weak continuous line has been recently discovered onboard Voyager 1 in the interstellar medium, whose origin raised two major questions. First, how can this line be produced by plasma quasi-thermal noise on the Voyager short antenna? Second, why do
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0527915077dd3db77723d46eac31cf6a
http://arxiv.org/abs/2202.04684
http://arxiv.org/abs/2202.04684
Akademický článek
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Akademický článek
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Autor:
J.A. Araneda, C. Beck, I.H. Cairns, J.F. Carbary, E.G.D. Cohen, K. Dialynas, M.A. Dopita, J. Dudík, E. Dzifčáková, L.A. Fisk, R. Gaelzer, G. Gloeckler, M. Kane, L.J. Kewley, S.M. Krimigis, G.S. Lakhina, B. Li, G. Livadiotis, R. Mace, B.H. Mauk, D.J. McComas, N. Meyer-Vernet, P.S. Moya, D.C. Nicholls, C.P. Paranicas, V. Pierrard, J.M. Schmidt, S. Singh, R.S. Sutherland, A.F. Viñas, P.H. Yoon, G.P. Zank
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::69be65ca6cd78cce1245492d73558b8c
https://doi.org/10.1016/b978-0-12-804638-8.01002-0
https://doi.org/10.1016/b978-0-12-804638-8.01002-0
Autor:
Donald G. Mitchell, P. Schippers, Ingrid Mann, N. André, M. Moncuquet, N. Meyer Vernet, Alain Lecacheux, William S. Kurth, S. Belheouane
Publikováno v:
The Astrophysical Journal
The Astrophysical Journal, American Astronomical Society, 2015, 806 (1), pp.77. ⟨10.1088/0004-637X/806/1/77⟩
The Astrophysical Journal, 2015, 806 (1), pp.77. ⟨10.1088/0004-637X/806/1/77⟩
The Astrophysical Journal, American Astronomical Society, 2015, 806 (1), pp.77. ⟨10.1088/0004-637X/806/1/77⟩
The Astrophysical Journal, 2015, 806 (1), pp.77. ⟨10.1088/0004-637X/806/1/77⟩
The solar system contains solids of all sizes, ranging from km-size bodies to nano-sized particles. Nanograins have been detected in situ in the Earth's atmosphere, near cometary and giant planet environments, and more recently in the solar wind at 1
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::28e3b9c15d041fe3cbebd3c906c29a84