Zobrazeno 1 - 10
of 18
pro vyhledávání: '"Charles Lue"'
Negative ions have been detected in abundance in recent years by spacecraft across the solar system. These detections were, however, made by instruments not designed for this purpose and, as such, significant uncertainties remain regarding the preval
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a419d469ae113b3be90993e36b60bbd5
Autor:
Andrey Divin, Douglas J. Hemingway, Jan Deca, Ian Garrick-Bethell, Mihaly Horanyi, Andrew R. Poppe, Charles Lue, Bertrand Lembège
Publikováno v:
Journal of Geophysical Research. Planets
Journal of Geophysical Research. Planets, Wiley-Blackwell, 2020, 125 (5), pp.e2019JE006219. ⟨10.1029/2019JE006219⟩
Journal of Geophysical Research. Planets, Wiley-Blackwell, 2020, 125 (5), pp.e2019JE006219. ⟨10.1029/2019JE006219⟩
International audience; The Reiner Gamma swirl is a prime location to investigate the lunar albedo patterns and their co‐location with magnetic anomalies. The precise relationship between impinging plasma and the swirl, and in particular, how these
Autor:
Mihaly Horanyi, Ian Garrick-Bethell, Andrew R. Poppe, Douglas J. Hemingway, Bertrand Lembège, Andrey Divin, Jan Deca, Charles Lue
The Reiner Gamma swirl is one of the most prominent albedo features on the lunar surface. Its modest spatial scales and structure allows fully kinetic modelling. The region therefore presents a prime location to investigate the lunar albedo patterns
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::999ed7300d3a3db555505af0364a2147
https://doi.org/10.5194/egusphere-egu2020-6186
https://doi.org/10.5194/egusphere-egu2020-6186
We investigate the dynamics of solar wind - Moon interaction by means of large-scale Particle-in-Cell (PIC) simulations in this study. Implicit moment PIC method and open boundaries are implemented in the code (iPIC3D) allowing to use large-scale dom
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a4901ee16eb8adb2749591f0efde02d9
https://doi.org/10.5194/egusphere-egu2020-18137
https://doi.org/10.5194/egusphere-egu2020-18137
Publikováno v:
J Geophys Res Space Phys
We study the scattering of solar wind protons off the lunar surface, using ion observations collected over 6 years by the ARTEMIS satellites at the Moon. We show the average scattered proton energy spectra, directional scattering distributions, and s
Publikováno v:
Communications Physics, Vol 1, Iss 1, Pp 1-8 (2018)
All lunar swirls are known to be co-located with crustal magnetic anomalies (LMAs). Not all LMAs can be associated with albedo markings, making swirls, and their possible connection with the former, an intriguing puzzle yet to be solved. By coupling
Publikováno v:
J Geophys Res Space Phys
A statistical investigation of five years of observations from the two-probe Acceleration, Reconnection, Turbulence, and Electrodynamics of Moon's Interaction with the Sun (ARTEMIS) mission reveals that strong compressional interactions occur infrequ
Autor:
Charles Lue, Stas Barabash, Martin Wieser, Mats Holmström, Shahab Fatemi, Andrew R. Poppe, Gregory T. Delory
Publikováno v:
Journal of Geophysical Research: Space Physics. 120:4719-4735
We present the results of the first local hybrid simulations (particle ions and fluid electrons) for the solar wind plasma interaction with realistic lunar crustal fields. We use a three-dimensiona ...
Publikováno v:
J Geophys Res Planets
Despite their small scales, lunar crustal magnetic fields are routinely associated with observations of reflected and/or backstreaming populations of solar wind protons. Solar wind proton reflection locally reduces the rate of space weathering of the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ab011f3bbae476f71db2927ecb2abd48
https://europepmc.org/articles/PMC7802739/
https://europepmc.org/articles/PMC7802739/
Effects of protons reflected by lunar crustal magnetic fields on the global lunar plasma environment
Autor:
Mats Holmström, Stas Barabash, Yoshifumi Futaana, Gabriella Stenberg, Michael R. Collier, Charles Lue, Shahab Fatemi
Publikováno v:
Journal of Geophysical Research: Space Physics. 119:6095-6105
Solar wind plasma interaction with lunar crustal magnetic fields is different than that of magnetized bodies like the Earth. Lunar crustal fields are, for typical solar wind conditions, not strong ...