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
  • [31] Cycle Variations in the Photospheric and Interplanetary Magnetic Field and Solar Wind Parameters
    I. A. Bilenko
    Geomagnetism and Aeronomy, 2019, 59 : 810 - 821
  • [32] On the variations of the solar wind magnetic field about the Parker spiral direction
    Borovsky, Joseph E.
    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2010, 115
  • [33] Magnetic Field Behavior in the Magnetosheath when the IMF Slightly Differs from the Solar Wind Velocity Vector
    Mezentsev, A. V.
    GEOMAGNETISM AND AERONOMY, 2013, 53 (03) : 307 - 312
  • [34] Influence of the solar-wind magnetic field on the Earth's magnetosheath turbulence behind the bow shock
    Barkhatov, N.A.
    Belliustin, N.S.
    Bougeret, J.
    Sakharov, S.Yu.
    Tokarev, Yu.V.
    Izvestiya Vysshikh Uchebnykh Zavedenij. Radiofizika, 2001, 44 (12): : 993 - 1003
  • [35] Magnetic field behavior in the magnetosheath when the IMF slightly differs from the solar wind velocity vector
    A. V. Mezentsev
    Geomagnetism and Aeronomy, 2013, 53 : 307 - 312
  • [36] Turbulent Cascade in the Magnetosheath Affected by the Solar Wind’s Plasma Turbulence
    L. S. Rakhmanova
    M. O. Riazantseva
    G. N. Zastenker
    Yu. I. Yermolaev
    I. G. Lodkina
    L. S. Chesalin
    Cosmic Research, 2019, 57 : 443 - 450
  • [37] Turbulent Cascade in the Magnetosheath Affected by the Solar Wind's Plasma Turbulence
    Rakhmanova, L. S.
    Riazantseva, M. O.
    Zastenker, G. N.
    Yermolaev, Yu. I.
    Lodkina, I. G.
    Chesalin, L. S.
    COSMIC RESEARCH, 2019, 57 (06) : 443 - 450
  • [38] MAGNETIC-FIELD CONFIGURATIONS ASSOCIATED WITH FAST SOLAR-WIND
    SHEELEY, NR
    WANG, YM
    SOLAR PHYSICS, 1991, 131 (01) : 165 - 186
  • [39] Turbulence and intermittency in the heliospheric magnetic field in fast and slow solar wind
    Yordanova, E.
    Balogh, A.
    Noullez, A.
    von Steiger, R.
    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2009, 114
  • [40] Composition variations in fast solar wind streams
    von Steiger, R
    Fiska, LA
    Gloeckler, G
    Schwadron, NA
    Zurbuchen, TH
    SOLAR WIND NINE, 1999, 471 : 143 - 146
12345