High spatial resolution microwave observations of the sun

Details High spatial resolution microwave observations of the sun High spatial resolution microwave observations of the sun

Oct 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985soph..100..491k&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 100, Oct. 1985, p. 491-514.

Astronomy and Astrophysics

Astronomy

13

Coronal Loops, Radio Astronomy, Radio Telescopes, Solar Corona, Solar Limb, Astronomical Maps, Cross Correlation, H Alpha Line, High Resolution, Least Squares Method, Solar Observatories, Spatial Resolution, Very Large Array (Vla)

Scientific paper

Some results are given that have been obtained at Maryland, based on observations with the Westerbork Synthesis Radio Telescope (WSRT) and the Very Large Array (VLA) on the quiet sun (supergranulation network and limb profile), active regions (sunspot-associated regions and coronal loops), and flaring regions. Topics covered include: observations of filaments; microwave active regions; determination of magnetic fields in the low corona; radio observations of coronal loops; and observations of flares with the VLA.

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