Multi-Spacecraft Observations of Magnetic Reconnection in the Solar Wind

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F13%3A10191865" target="_blank" >RIV/00216208:11320/13:10191865 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1063/1.4811012" target="_blank" >http://dx.doi.org/10.1063/1.4811012</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1063/1.4811012" target="_blank" >10.1063/1.4811012</a>

Result language
angličtina
Original language name
Multi-Spacecraft Observations of Magnetic Reconnection in the Solar Wind
Original language description
We discuss magnetic reconnection occurring at the boundary between the interplanetary coronal mass ejection sheath and magnetic cloud-like structure (MCL). Multi-spacecraft observations of this event allow us to conclude that such type of reconnection persists more than 50 minutes and the reconnection exhaust can be detected over a distance larger than 130 R-E. The analysis of the event suggests that the observed velocity of the accelerated flow inside the exhaust decreases with the distance from the reconnection X-line.
Czech name
—
Czech description
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Project
<a href="/en/project/GA205%2F09%2F0112" target="_blank" >GA205/09/0112: Study of the regions associated with magnetopause reconnection</a><br>
Continuities
Z - Vyzkumny zamer (s odkazem do CEZ)<br>S - Specificky vyzkum na vysokych skolach<br>I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2013
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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