Interaction of Phobos with the Solar Wind Plasma

Details Interaction of Phobos with the Solar Wind Plasma Interaction of Phobos with the Solar Wind Plasma

Sep 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001cosre..39..446m&link_type=abstract

Cosmic Research, v. 39, Issue 5, p. 446-452 (2001).

Physics

2

Scientific paper

The interaction of Phobos with the solar wind is considered both theoretically and using the experimental data of the FGMM magnetometer that were obtained in the course of the Phobos-2mission. It is demonstrated that the ions serving as a source of excitation of magnetosonic waves can be accumulated around Phobos. Examination of the magnetometer data has shown that the observed effects of a local decrease of the magnetic field near the Phobos orbit correspond to magnetosonic waves. Observation of these effects depends on the geometry of an experiment.

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