VLA observations of coronal bright points at 6 and 20 CM wavelengths

Details VLA observations of coronal bright points at 6 and 20 CM wavelengths VLA observations of coronal bright points at 6 and 20 CM wavelengths

Dec 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986nascp2442..349k&link_type=abstract

In NASA. Goddard Space Flight Center Coronal and Prominence Plasmas p 349-351 (SEE N87-20871 13-92)

Physics

1

Brightness Temperature, Faculae, Solar Corona, Solar Granulation, Thermal Plasmas, Magnetic Signatures, Spacelab Payloads, Spatial Resolution, Spectroheliographs, Very Large Array (Vla)

Scientific paper

Prior to and during the Spacelab-2 operation, observations were made at 6 and 20 cm of solar coronal bright points, using the Very Large Array (VLA) in the C-configuration. The ultraviolet coverage ranged from 200 to 18,000 wavelengths. The maps were convolved with beams of 18 x 18 inches at 20 km and 4 x 4 inches at 6 cm. Only the preliminary results from July 15 and July 31, 1985 observations.

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