A comparison of synchronous observations of a prominence in the radio and optical regions

Details A comparison of synchronous observations of a prominence in the radio and optical regions A comparison of synchronous observations of a prominence in the radio and optical regions

Jan 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984velen......107a&link_type=abstract

Leningradskii Universitet, Vestnik, Matematika, Mekhanika, Astronomiia (ISSN 0024-0850), Jan. 1984, p. 107-109. In Russian.

Astronomy and Astrophysics

Astronomy

Astronomical Photometry, Brightness Distribution, Radio Astronomy, Solar Prominences, Centimeter Waves, H Alpha Line, Optical Measurement, Solar Eclipses, Solar Radio Emission

Scientific paper

The observations were made on July 31, 1981. The photometric measurements were obtained in the form of a field of values for the intensity along the prominence. For purposes of comparison with the radio data, a determination was made of the flux in the H-alpha line, as though being observed together with a radio telescope beam. In interpreting the results, it is pointed out that the separate parts of the prominence probably possessed significant radial velocities and that as a consequence the radiation of hydrogen in observations in the band at 0.25 A may not be taken into account.

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