Title of article
Substorm and storm time ionospheric particle flux at the Moon while in the terrestrial magnetosphere
Author/Authors
Harnett، نويسنده , , Erika M. and Cash، نويسنده , , Michele and Winglee، نويسنده , , Robert M.، نويسنده ,
Issue Information
روزنامه با شماره پیاپی سال 2013
Pages
10
From page
218
To page
227
Abstract
The Moon spends 20% of its orbit within the terrestrial magnetosphere. During this time it experiences a flux of ions from the Earth, which can be accelerated within the magnetosphere prior to impacting the Moon. Both 3D multi-fluid simulations and particle tracking were used to study the lunar environment while the Moon is inside the magnetosphere and quantify the energy and flux of ionospheric ions at lunar orbits for times ranging from moderate substorms to severe storms. The results from the fluid simulations indicate that during storms, the flux of ionospheric oxygen ions to the Moon can increase by two orders of magnitude and the bulk of those oxygen ions have energies up to 100s of keV. Particle tracking indicates that the peak energy of particles in the tail of the distribution approaches 1 MeV for the most intense storms, as particles from the ring current can be lost downtail to lunar orbits. Periods of increased flux of ionospheric particles intercepted by the Moon over geologic time periods would have played a role in weathering of the lunar surface and delivery of water components to the surface.
Keywords
moon , Magnetospheres , Earth , solar wind
Journal title
Icarus
Serial Year
2013
Journal title
Icarus
Record number
2379864
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