| Issue |
EAS Publications Series
Volume 55, 2012
4th French-Chinese Meeting on Solar Physics - Understanding Solar Activity: Advances and Challenges
|
|
|---|---|---|
| Page(s) | 327 - 334 | |
| Section | CMEs and Space Weather | |
| DOI | https://doi.org/10.1051/eas/1255045 | |
| Published online | 27 June 2012 | |
M. Faurobert, C. Fang and T. Corbard (eds)
EAS Publications Series, 55 (2012) 327-334
Observation of magnetic reconnection at the turbulent leading edge of an interplanetary coronal mass ejection
1
Observatoire de Paris, LESIA, CNRS, 92195
Meudon,
France
e-mail: Abraham.Chian@obspm.fr
2
National Institute for Space Research (INPE) and World Institute
for Space Environment Research (WISER), São José dos Campos-SP
12227-010,
Brazil
3
Institute of Aeronautical Technology (ITA),
São José dos Campos-SP
12228-900,
Brazil
e-mail: pablocus@gmail.com
Magnetic Cloud Boundary Layer (MCBL) is formed by the interaction between a magnetic cloud ejected by the Sun and the ambient solar wind, which may be linked to the outer loops of an Interplanetary Coronal Mass Ejection (ICME) and often display the properties of magnetic reconnection. We study the relation between current sheets, turbulence, and magnetic reconnection at the leading edge of an ICME intercepted by the four Cluster spacecraft in the solar wind, upstream of the Earth’s bow shock, on 2005 January 21. We obtain the observational evidence of a fully-developed magnetic turbulence in the vicinity of two current sheets at the leading edge of ICME. Each current sheet shows the signatures of magnetic reconnections with oppositely propagating Alfven waves and jets. The current density of bifurcated current sheets is computed by the curlometer technique using multi-spacecraft data.
© EAS, EDP Sciences 2012