Charged particles close to the Mars surface

Details Charged particles close to the Mars surface Charged particles close to the Mars surface

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf.1194r&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.1194

Computer Science

Scientific paper

One way to address the Martian crustal magnetization is to use the classical source models, where the field created by a volume of a magnetized material is compared with the observed one. These source models allow introducing additional constraints related to the available information of the magnetic field. In this context, our goal is to find the relevant features of the charged particle dynamics at low altitudes in the Martian atmosphere. To this purpose, the motion of different charged particles (e-, p+ and 4He) moving in different uniformly magnetized sources has been analyzed. To complete this study, the gravitational field has been included in all the equations. To a first approximation, we have assumed a constant gravitational field and finally, a non-uniform gravitational field dependent on altitude has been modeled. The dynamics of the charged particles has been studied numerically in to coordinates representations, (x,y,z) and (,z) where =(x2 + y2)1/2.

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