INDIRECT EVIDENCES FOR A GAS DUST TORUS ALONG THE PHOBOS ORBIT

被引:67
作者
DUBININ, EM
LUNDIN, R
PISSARENKO, NF
BARABASH, SV
ZAKHAROV, AV
KOSKINEN, H
SCHWINGENSHUH, K
YEROSHENKO, YG
机构
[1] SWEDISH INST SPACE PHYS,S-98128 KIRUNA,SWEDEN
[2] FINNISH METEOROL INST,SF-00101 HELSINKI,FINLAND
[3] AUSTRIAN SPACE RES INST,A-8010 GRAZ,AUSTRIA
[4] ACAD SCI USSR,INST TERR MAGNETIZM IONOSPHERE & RADIO WAVE PROPAGAT,TROITSK,USSR
关键词
D O I
10.1029/GL017i006p00861
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Observations from the PHOBOS‐2 space‐craft of plasma and magnetic field effects in the solar wind near Mars suggest that a neutral gas (dust?)torus/ring resides along the orbit of the Martian satellite Phobos. Magnetic ‘cavities’(strong decreases of the magnetic field strength) coincident with strong plasma density increases (up to a factor of ten) are observed during the first elliptic transition orbits when the spacecraft approached the Phobos orbits. The characteristic transverse dimension of the structures along the spacecraft orbit is in the range 100–1000 km, ‘Torus effects’ also have characteristics similar to the formation of a bow shock with increases of plasma density and ion temperature, and a characteristic deflection of the ion flow. This suggests a rather strong interaction between the solar wind plasma and plasma near Phobos orbit. The interaction appears quite similar to that of the solar wind with a comet. The oiitgassing of matter from Phobos (and Deimos) is also suggested by plasma observations in the wake/tail of the Martian satellites. Altogether, our observations imply that a neutral gas cloud—possibly also associated with a faint dust ring—exists along the Phobos orbit. Copyright 1990 by the American Geophysical Union.
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收藏
页码:861 / 864
页数:4
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