Fast solar wind plasma and magnetic field variations in the magnetosheath

被引：0
|
作者：
Zastenker, GN [1 ]
Nozdrachev, MN
Safránková, J
Nemecek, Z
Paularena, KI
Lazarus, AJ
Lepping, RP
Mukai, T
机构：
[1] Russian Acad Sci, Space Res Inst, Moscow, Russia
[2] Charles Univ, Fac Math & Phys, Prague, Czech Republic
[3] MIT, Ctr Space Res, Cambridge, MA 02139 USA
[4] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[5] Inst Space & Astronaut Sci, Sagamihara, Kanagawa 229, Japan
来源：
CZECHOSLOVAK JOURNAL OF PHYSICS | 1999年 / 49卷 / 4A期
关键词：
D O I：
暂无
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
The results of experimental study of plasma and magnetic field fast variations in the magnetosheath and their comparison with the gasdynamic model are presented. These variations on the scale of minutes or tens of minutes are several times larger than simultaneous solar wind plasma and interplanetary magnetic field (IMF) variations and cannot be explained by the motion of the magnetosheath as whole. The level of variations does not depend on the angle between the IMF vector and the normal to the bow shock (theta(BN)).
引用
收藏
页码：579 / 590
页数：12
相关论文
共 50 条
  • [21] Search for plasma and magnetic field cavities in magnetosheath
    Türk, F
    Kaymaz, Z
    Sibeck, DG
    PLASMA PROCESSES IN THE NEAR-EARTH SPACE: INTERBALL AND BEYOND, 2003, 31 (05): : 1455 - 1462
  • [22] Distribution of magnetic field components in the solar wind plasma
    Padhye, NS
    Smith, CW
    Matthaeus, WH
    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2001, 106 (A9) : 18635 - 18650
  • [23] Small-scale ion flux and magnetic field fluctuations in solar wind, foreshock and magnetosheath
    Shevyrev, N. N.
    Jian, Du
    Zastenker, G. N.
    Chi, Wang
    Eiges, P. E.
    CHINESE PHYSICS, 2007, 16 (05): : 1477 - 1487
  • [24] SIMULTANEOUS SOLAR WIND - MAGNETOSHEATH PLASMA MEASUREMENTS BY A PAIR OF SATELLITES
    GILBERT, HE
    BAME, SJ
    OGILVIE, KW
    TRANSACTIONS-AMERICAN GEOPHYSICAL UNION, 1971, 52 (11): : 913 - &
  • [25] A statistical study of magnetic field fluctuations in the dayside magnetosheath and their dependence on upstream solar wind conditions
    Dimmock, A. P.
    Nykyri, K.
    Pulkkinen, T. I.
    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2014, 119 (08)
  • [26] Coronal magnetic field topology and source of fast solar wind
    Guhathakurta, M
    Sittler, E
    Fisher, R
    McComas, D
    Thompson, B
    GEOPHYSICAL RESEARCH LETTERS, 1999, 26 (19) : 2901 - 2904
  • [27] Multispacecraft measurements of plasma and magnetic field variations in the magnetosheath:: Comparison with Spreiter models and motion of the structures
    Zastenker, GN
    Nozdrachev, MN
    Nemecek, Z
    Safránkova, J
    Paularena, KI
    Richardson, JD
    Lepping, RP
    Mukai, T
    PLANETARY AND SPACE SCIENCE, 2002, 50 (5-6) : 601 - 612
  • [28] Rotation of the magnetic field in Earth's magnetosheath by bulk magnetosheath plasma flow
    Longmore, M
    Schwartz, SJ
    Lucek, EA
    ANNALES GEOPHYSICAE, 2006, 24 (01) : 339 - 354
  • [29] Cycle Variations in the Photospheric and Interplanetary Magnetic Field and Solar Wind Parameters
    Bilenko, I. A.
    GEOMAGNETISM AND AERONOMY, 2019, 59 (07) : 810 - 821
  • [30] Geosynchronous magnetic field temporal response to solar wind and IMF variations
    Wing, S
    Sibeck, DG
    Wiltberger, M
    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2002, 107 (A8)
12345