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

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

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...

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Veröffentlicht in:Advances in space research 2009-02, Vol.43 (4), p.495-498
Hauptverfasser: Mitsakou, E., Babasidis, G., Moussas, X.
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Sprache:eng
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Coronal mass ejections
Magnetic field
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container_title Advances in space research
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creator Mitsakou, E.
Babasidis, G.
Moussas, X.
description 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.
doi_str_mv 10.1016/j.asr.2008.08.003
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subjects Coronal mass ejections
Magnetic field
title Interplanetary coronal mass ejections during the descending cycle 23: Sheath and ejecta properties comparison
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