A study of the magnetic evolution of active regions and its relation to solar flares

Details A study of the magnetic evolution of active regions and its relation to solar flares A study of the magnetic evolution of active regions and its relation to solar flares

Jan 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ucnr.rept.....c&link_type=abstract

Final Report, 21 Apr. 1981 - 20 Jul. 1982 California State Univ., Northridge.

Physics

Solar Flares, Solar Magnetic Field, Solar Spectra, Evolution (Development), Line Spectra, Magnesium, Magnetic Variations

Scientific paper

Observations of solar magnetic fields and associated activity, obtained
with a Magnesium b-line (5172 A) Etalon Filter, are described.
Particular emphasis is placed on flares visible in the wings of the
Magnesium line; such flare structures are of small size (4-6 arcsec) and
their intensities are strongly correlated with soft X-ray fluxes.

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