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Paper: Chromospheric Magnetic Reconnection
Volume: 369, New Solar Physics with Solar-B Mission
Page: 243
Authors: Chae, J.
Abstract: 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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