Physics
Scientific paper
Feb 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993jgr....98.1303v&link_type=abstract
Journal of Geophysical Research (ISSN 0148-0227), vol. 98, no. A2, p. 1303-1309.
Physics
35
Magnetopause, Mars Atmosphere, Mass Spectrometers, Shock Waves, Solar Protons, Solar Wind, Circular Orbits, Geomagnetism, Planetary Magnetotails, Satellite Orbits, Mars, Magnetosphere, Magnetopause, Bowshock, Solar Wind, Interaction, Pressure, Spacecraft Observations, Phobos 2 Mission, Taus Instrument, Spectrometry, Position (Location), Spectra, Protons, Magnetotail, Thickness, Magnetic Field, Magma Instrument, Analysis
Scientific paper
Results of the first quantitative studies of the variability of the Martian magnetopause are presented. On the basis of measurements of the 3D solar wind proton spectra measured by the TAUS spectrometer on board Phobos 2 in its 56 circular orbits, the location of the Martian magnetopause is studied as a function of solar wind ram pressure and is compared with that of the Martian bow shock. In the power-law expression showing the dependence of the Martian magnetotail thickness D on the solar wind ram pressure: D is approximately equal to (pv-squared) exp -1/k, the power index (k) was about 5.9 +/- 0.5. From the close coincidence of this index with k = 6 for a dipole geomagnetic field, and the large aeromagnetotail thickness compared with the planetary diameter, it is suggested that an intrinsic dipole magnetic field is likely to be an important factor in the solar wind interaction with Mars.
Apáthy I.
Gringauz K. I.
Kotova Galina A.
Livi Stefano S.
Remizov A. P.
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