Magnetic field reconnection in the flare of 18:28 UT 1975 August 10

Details Magnetic field reconnection in the flare of 18:28 UT 1975 August 10 Magnetic field reconnection in the flare of 18:28 UT 1975 August 10

Dec 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...210l.149c&link_type=abstract

Astrophysical Journal, vol. 210, Dec. 15, 1976, pt. 2, p. L149-L151.

Astronomy and Astrophysics

Astrophysics

5

Magnetic Effects, Magnetic Field Reconnection, Magnetic Flux, Solar Flares, Solar Magnetic Field, Chromosphere, H Alpha Line, Magnetic Field Configurations, Photosphere, Solar X-Rays

Scientific paper

The letter discusses observations of the cited flare made with the Sacramento Peak Observatory 512-diode array, which simultaneously measures photospheric magnetic fields, photospheric and chromospheric velocities, and chromospheric brightness in several lines. The observations suggest triggering of the flare by emergence of new magnetic flux, as well as the geometry of the reconnected field during the flare. Implications of the present observations regarding the site of the initial instability are discussed as well as the relationship to X-ray observations.

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