Interplanetary coronal mass ejections during the descending cycle 23: Sheath and ejecta properties comparison

被引：6
|
作者：
Mitsakou, E. [1 ]
Babasidis, G. [1 ]
Moussas, X. [1 ]
机构：
[1] Univ Athens, Sect Astrophys Astron & Mech, Fac Phys, GR-15783 Athens, Greece
来源：
ADVANCES IN SPACE RESEARCH | 2009年 / 43卷 / 04期
关键词：
Coronal mass ejections; Magnetic field; MAGNETIC CLOUDS; SOLAR-WIND; SOLAR-CYCLE-23; ORIGIN; MAXIMUM; PLASMA; STORMS; SHOCK; 1-AU; AU;
D O I：
10.1016/j.asr.2008.08.003
中图分类号：
V [航空、航天];
学科分类号：
08 ; 0825 ;
摘要：
We have used Omniweb data in order to identify the sheath and the ejecta boundaries of 67 shock-driving interplanetary coronal mass ejections during the time period 2003-2006. We examine and compare their statistical properties (speed, magnetic field strength, proton density and temperature, proton plasma beta), with those of the typical solar wind. We also calculate their passage time and radial width. We study the correlation between the ejecta and sheath characteristics. (C) 2008 COSPAR. Published by Elsevier Ltd. All rights reserved.
引用
收藏
页码：495 / 498
页数：4
相关论文
共 50 条
  • [31] Coronal mass ejections and active prominences relationship during solar cycle 23
    Lara, Alejandro
    Caballero, Rogelio
    Mendoza, Eduardo
    FIFTY YEARS OF ROMANIAN ASTROPHYSICS, 2007, 895 : 153 - +
  • [32] Statistical analysis of interplanetary coronal mass ejections and their geoeffectiveness during the solar cycles 23 and 24
    P. Alexakis
    H. Mavromichalaki
    Astrophysics and Space Science, 2019, 364
  • [33] Filaments disappearance in relation to coronal mass ejections during the solar cycle 23
    Mawad, R.
    Shaltout, Mosalam
    Yousef, M.
    Yousef, S.
    Ewaida, M.
    ADVANCES IN SPACE RESEARCH, 2015, 55 (02) : 688 - 695
  • [34] Statistical analysis of interplanetary coronal mass ejections and their geoeffectiveness during the solar cycles 23 and 24
    Alexakis, P.
    Mavromichalaki, H.
    ASTROPHYSICS AND SPACE SCIENCE, 2019, 364 (11)
  • [35] Kinetic properties of coronal mass ejections corrected for the projection effect in Cycle 23
    Gao, Peng-Xin
    Li, Ke-Jun
    Li, Qi-Xiu
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2009, 394 (02) : 1031 - 1036
  • [36] Properties of interplanetary coronal mass ejections at one AU during 1995-2004
    Jian, L.
    Russell, C. T.
    Luhmann, J. G.
    Skoug, R. M.
    SOLAR PHYSICS, 2006, 239 (1-2) : 393 - 436
  • [37] Proton Temperature Anisotropy within the Interplanetary Coronal Mass Ejections Sheath at 1 au
    Shaikh, Zubair I.
    Raghav, Anil N.
    Vasko, Ivan Y.
    ASTROPHYSICAL JOURNAL LETTERS, 2023, 955 (01)
  • [38] Alfven Ion Cyclotron Waves in Sheath Regions Driven by Interplanetary Coronal Mass Ejections
    Ala-Lahti, Matti
    Kilpua, Emilia K. J.
    Soucek, Jan
    Pulkkinen, Tuija, I
    Dimmock, Andrew P.
    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2019, 124 (06) : 3893 - 3909
  • [39] Minimum Variance Analysis of Interplanetary Coronal Mass Ejections Around Solar Cycle 23 Maximum (1998–2002)
    E. Echer
    W. D. Gonzalez
    M. V. ALVES
    Solar Physics, 2006, 233 : 249 - 263
  • [40] The true dimensions of interplanetary coronal mass ejections
    Russell, CT
    Mulligan, T
    STRUCTURE, ENERGETICS AND DYNAMICS OF THE CORONA AND THE HELIOSPHERE DURING THE RISING PHASE OF THE 23RD SOLAR CYCLE, 2002, 29 (03): : 301 - 306
12345