Large and fast variations of parameters in the magnetosheath: 3. Amplitudes and transverse profiles of low and high frequency variations of the plasma and magnetic field

被引:1
|
作者
Shevyrev, NN
Zastenker, GN
Safrankova, J
Nemecek, Z
Gaiosh, M
Richardson, JD
机构
[1] Russian Acad Sci, Inst Space Res, Moscow 117997, Russia
[2] Charles Univ, Fac Math & Phys, Prague, Czech Republic
[3] MIT, Ctr Space Res, Cambridge, MA 02139 USA
基金
美国国家科学基金会; 俄罗斯基础研究基金会;
关键词
D O I
10.1023/A:1019842327538
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
We present the results of experimental studies of high frequency (with periods of seconds and tens of seconds) and low frequency (with periods of minutes and tens of minutes) large variations of the ion flux and magnetic field magnitude in the magnetosheath. It is shown that, on average, the relative amplitudes of these variations are approximately two times higher than similar values characteristic for the undisturbed solar wind. The averaged spatial profile of these values and their variations across the magnetosheath is obtained, as are the dependencies of normalized plasma fluxes and their variations on the place of entrance of a given plasma element into the magnetosheath. Using one particular example, a good coincidence between the time profiles of ion fluxes measured aboard two spacecraft separated by a distance of 10R(E) along the magnetosheath is demonstrated.
引用
收藏
页码:335 / 346
页数:12
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