Chromospheric Magnetic Reconnection

Details Chromospheric Magnetic Reconnection Chromospheric Magnetic Reconnection

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..369..243c&link_type=abstract

New Solar Physics with Solar-B Mission ASP Conference Series, Vol. 369, proceedings of the conference held 8-11 November, 2005 a

Physics

2

Scientific paper

There has been increasing observational evidence that magnetic reconnection often occurs in the low atmosphere of the sun. I will present a brief review of our recent observational results on canceling magnetic features in the photosphere and jet-like events in the chromosphere and discuss the expected physical properties of magnetic reconnection occurring in the photosphere and chromosphere based on an adiabatic current sheet model of Sweet-Parker type. A special attention is paid to the temperature-speed relation in jet-like events in the chromosphere, and the need of anomalous resistivity in the model of chromospheric magnetic reconnection.

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