Energetic protons at Mars: interpretation of SLED/Phobos-2 observations by a kinetic model
Mars has neither a significant global intrinsic magnetic field nor a dense atmosphere. Therefore, solar energetic particles (SEPs) from the Sun can penetrate close to the planet (under some circumstances reaching the surface). On 13 March 1989 the SLED instrument aboard the Phobos-2 spacecraft r...
Main Authors: | E. Kallio, S. McKenna-Lawlor, M. Alho, R. Jarvinen, S. Dyadechkin, V. V. Afonin |
---|---|
Format: | Article |
Language: | English |
Published: |
Copernicus Publications
2012-11-01
|
Series: | Annales Geophysicae |
Online Access: | https://www.ann-geophys.net/30/1595/2012/angeo-30-1595-2012.pdf |
Similar Items
-
Trajectory Optimization and Control Applied to Landing Maneuvers on Phobos from Mars-Phobos Distant Retrograde Orbits
by: Vittorio Baraldi, et al.
Published: (2023-07-01) -
Atmospheric contribution to the dissipation of the gravitational tide of Phobos on Mars
by: Thayalan, Vid
Published: (2009) -
Surface environment of Phobos and Phobos simulant UTPS
by: Hideaki Miyamoto, et al.
Published: (2021-12-01) -
Lessons from PHOBOS
by: Busza, Wit
Published: (2010) -
Ultraviolet and visible reflectance spectra of Phobos and Deimos as measured by the ExoMars-TGO/Nomad-UVIS spectrometer
by: Mason, JP, et al.
Published: (2023)