Sharp boundaries of solar wind plasma structures and an analysis of their pressure balance

被引：13
|
作者：
Riazantseva, MO
Khabarova, OV
Zastenker, GN
Richardson, JD
机构：
[1] Russian Acad Sci, Space Res Inst, Moscow 117997, Russia
[2] Moscow MV Lomonosov State Univ, Skobeltsyn Inst Nucl Phys, Moscow 119899, Russia
[3] Russian Acad Sci, Inst Terr Magnetism Ionosphere & Radio Wave Propa, Troitsk, Moscow Oblast, Russia
[4] MIT, Ctr Space Res, Cambridge, MA 02139 USA
来源：
COSMIC RESEARCH | 2005年 / 43卷 / 03期
基金：
俄罗斯基础研究基金会; 美国国家科学基金会;
关键词：
Magnetic Field; Solar Wind; Time Resolution; Simultaneous Measurement; Typical Condition;
D O I：
10.1007/s10604-005-0030-8
中图分类号：
V [航空、航天];
学科分类号：
08 ; 0825 ;
摘要：
This work is devoted to studying the sharp boundaries of small-scale structures of the solar wind according to the data of measurements with high time resolution onboard the INTERBALL-1 satellite and simultaneous measurements of the WIND spacecraft. Such issues as the character of change of various plasma and magnetic field parameters on these boundaries, the duration of boundary passage and the balance of the total (thermal plus magnetic) pressure on the boundaries of the structures are considered. On the basis of the vast statistical material available, the typical conditions in the solar wind are investigated, in which such sharp boundaries are observed.
引用
收藏
页码：157 / 164
页数：8
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