On the Magnetic Energy Avalanche in the Solar Atmosphere

Details On the Magnetic Energy Avalanche in the Solar Atmosphere On the Magnetic Energy Avalanche in the Solar Atmosphere

Jun 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001ap%26ss.277..153r&link_type=abstract

Astrophysics and Space Science, v. 277, Issue 1/2, p. 153-156 (2001).

Astronomy and Astrophysics

Astrophysics

Scientific paper

We discuss a mechanism of energy production associated with the acoustic and MHD shocks produced by colliding and reconnecting flux tubes and present the observational results showing a connection between the dynamic changes in the photosphere and the high velocity and heating events in the transition region. We suggest that these processes may provide a constant energy supply for the origin of the fast wind and help to advance studies of coronal dynamics.

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