ORIGIN AND MAINTENANCE OF THE OXYGEN TORUS IN SATURNS MAGNETOSPHERE

被引:22
作者
MORFILL, GE
HAVNES, O
GOERTZ, CK
机构
[1] MAX PLANCK INST EXTRATERR PHYS, W-8046 GARCHING, GERMANY
[2] UNIV TROMSO, INST MATH & PHYS SCI, N-9001 TROMSO, NORWAY
[3] UNIV IOWA, DEPT PHYS & ASTRON, IOWA CITY, IA 52242 USA
关键词
D O I
10.1029/93JA00308
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Observations of thermal ions in Saturn's inner magnetosphere suggest distributed local sources rather than diffusive mass loading from a source located further out. We suggest that the plasma is produced and maintained mainly by ''self-sputtering'' of E ring dust. Sputtered particles are ''picked up'' by the planetary magnetospheric field and accelerated to corotation energies (of the order of 8 eV/amu). The sputter yield for oxygen on ice at, for example, 120 eV is approximately 5, which implies that an avalanche of self-sputtering occurs. The plasma density is built up until it is balanced by local losses, presumably pitch angle scattering into the loss cone and absorption in the planet's ionosphere. The plasma density determines the distribution of dust in the E ring through plasma drag. Thus a feedback mechanism between the plasma and the E ring dust is established. The model accounts for the principal plasma observations and simultaneously the radial optical depth profile of the E ring.
引用
收藏
页码:11285 / 11297
页数:13
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