On the Rapid Variations of Solar Magnetic Fields

Details On the Rapid Variations of Solar Magnetic Fields On the Rapid Variations of Solar Magnetic Fields

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003basi...31..299v&link_type=abstract

Bulletin of the Astronomical Society of India, vol. 31, p.299-301

Astronomy and Astrophysics

Astronomy

Sun, Mhd, Photosphere

Scientific paper

We report on the rapid variations of solar magnetic fields that appear to be enhanced significantly above the background variability, at a few locations within the solar active regions, as observed with the Michelson Doppler Imager (MDI) on board the SOHO spacecraft. The pressure fluctuations estimated to arise from this variability far exceed the general level of acoustic pressure fluctuations. The equivalent mechanical flux that could be generated from these rapid magnetic variations is more than adequate for the heating of the active region chromosphere and corona.

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