Determination of coronal magnetic fields from vector magnetograms

Details Determination of coronal magnetic fields from vector magnetograms Determination of coronal magnetic fields from vector magnetograms

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992saic.reptq....m&link_type=abstract

Semiannual Progress Report, 30 Jun. - 31 Dec. 1992 Science Applications International Corp., San Diego, CA.

Statistics

Applications

Force-Free Magnetic Fields, Mathematical Models, Solar Corona, Solar Magnetic Field, Boundary Conditions, Magnetic Signatures, Magnetohydrodynamics, Photosphere

Scientific paper

The determination of coronal magnetic fields from vector magnetograms, including the development and application of algorithms to determine force-free coronal fields above selected observations of active regions is studied. Two additional active regions were selected and analyzed. The restriction of periodicity in the 3-D code which is used to determine the coronal field was removed giving the new code variable mesh spacing and is thus able to provide a more realistic description of coronal fields. The NOAA active region AR5747 of 20 Oct. 1989 was studied. A brief account of progress during the research performed is reported.

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