Latitudinal density dependence of magnetic field lines inferred from Polar plasma wave data

被引:64
作者
Goldstein, J
Denton, RE
Hudson, MK
Miftakhova, EG
Young, SL
Menietti, JD
Gallagher, DL
机构
[1] Dartmouth Coll, Dept Phys & Astron, Wilder Lab 6127, Hanover, NH 03755 USA
[2] Univ Iowa, Dept Phys & Astron, Iowa City, IA 52242 USA
[3] NASA, George C Marshall Space Flight Ctr, Huntsville, AL 35812 USA
关键词
D O I
10.1029/2000JA000068
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Using observations of the electron density n(e) based on measurement of the upper hybrid resonance frequency by the Polar spacecraft Plasma Wave Instrument, we have examined the radial density dependence along field lines in the outer plasmasphere and the near plasma trough. Our technique depends, on the fact that Polar crosses particular L values at two different points with different radial distance R. Sampled L values range from 2.5 to 6.3. In our plasmaspheric data set (n(e) greater than or equal to 100 cm(-3)) we find that, on average, n(e) is flat along field lines from the equator up to the latitudes sampled by Polar (R greater than or similar to 2 R-E) In the plasma trough data set (n(e) < 100 cm(-3)) there is, on average, a mild radial dependence n(e) <proportional to> R-1.7.
引用
收藏
页码:6195 / 6201
页数:7
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