An Evaluation of Possible Mechanisms for Anomalous Resistivity in the Solar Corona

A wide variety of transient events in the solar corona seem to require explanations that invoke fast reconnection. Theoretical models explaining fast reconnection often rely on enhanced resistivity. We start with data derived from observed reconnection rates in solar flares and seek to reconcile the...

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Veröffentlicht in:	Solar physics 2007-07, Vol.243 (2), p.163-169
Hauptverfasser:	Singh, K. A. P., Subramanian, Prasad
Format:	Artikel
Sprache:	eng
Schlagworte:	Solar flares Solar physics Sun
Online-Zugang:	Volltext
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