Abstract A model is developed to study the ionospheric ion flux distribution along magnetic force lines in Martian magnetosphere and the influence of Martian intrinsic moment on the distribution. It is discovered that the intrinsic moment has significant influence on the O+ ion flux distribution that a lower flux in the magnetotail will be associated with a stronger intrinsic moment. According to the theoretical result and the observed data on the ion flux which is about 7.6×106 cm−2 s−1 in the Martian magnetotail, the deduced Martian moment is about 2×1021 G cm3. This agrees well with the most recent data obtained by MAG/ER on the Mars Global Surveyor spacecraft
The effect of the Martian crustal magnetic field on ion escape is the focus of considerable interest...
International audienceThis work presents a massive statistical analysis of the ion flows in the Mart...
International audienceAnalysis of MAVEN/STATIC observations in the Martian upper atmosphere, bounded...
International audienceWe present the effects of the local magnetic field configurations on ions prec...
Abstract: Ion escape from the atmosphere to space is one of the most likely reasons to account for t...
Historically, studying the Martian ionosphere has been difficult due to the lack of dedicated instru...
International audienceDirect interaction between the solar wind (SW) and the Martian upper atmospher...
Analysis of Mars Atmosphere and Volatile Evolution (MAVEN)/Supra‐Thermal And Thermal Ion Composition...
Based on a recent model of the Martian atmosphere/exosphere and a model of the magnetic field and so...
Without the protection of a global magnetic field, erosion of the Martian ionosphere by the solar wi...
International audienceThe interplanetary magnetic field (IMF) embedded in the solar wind interacts w...
International audienceEnergetic O+ and O2+ ions with energies of up to a few hundred eV are observed...
The effect of the Martian crustal magnetic field on ion escape is the focus of considerable interest...
International audienceThis work presents a massive statistical analysis of the ion flows in the Mart...
International audienceAnalysis of MAVEN/STATIC observations in the Martian upper atmosphere, bounded...
International audienceWe present the effects of the local magnetic field configurations on ions prec...
Abstract: Ion escape from the atmosphere to space is one of the most likely reasons to account for t...
Historically, studying the Martian ionosphere has been difficult due to the lack of dedicated instru...
International audienceDirect interaction between the solar wind (SW) and the Martian upper atmospher...
Analysis of Mars Atmosphere and Volatile Evolution (MAVEN)/Supra‐Thermal And Thermal Ion Composition...
Based on a recent model of the Martian atmosphere/exosphere and a model of the magnetic field and so...
Without the protection of a global magnetic field, erosion of the Martian ionosphere by the solar wi...
International audienceThe interplanetary magnetic field (IMF) embedded in the solar wind interacts w...
International audienceEnergetic O+ and O2+ ions with energies of up to a few hundred eV are observed...
The effect of the Martian crustal magnetic field on ion escape is the focus of considerable interest...
International audienceThis work presents a massive statistical analysis of the ion flows in the Mart...
International audienceAnalysis of MAVEN/STATIC observations in the Martian upper atmosphere, bounded...