Statistical comparison of radio granulation and the calcium chromospheric network

Details Statistical comparison of radio granulation and the calcium chromospheric network Statistical comparison of radio granulation and the calcium chromospheric network

Aug 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989azh....66..822g&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 66, July-Aug. 1989, p. 822-831. In Russian.

Astronomy and Astrophysics

Astronomy

Solar Cycles, Solar Granulation, Solar Radio Emission, Autocorrelation, Birefringent Filters, Periodic Variations, Radio Telescopes, Spectrum Analysis, Statistical Analysis

Scientific paper

Statistical results are presented from a study of simultaneous observations of radio granulation and the chromospheric network (Ca II K birefringent filter). The observations were made on July 21 and 28, and August 3, 1976, during a minimum phase of solar activity. The structures of radio granulation on a spatial scale of 44 and 122 arcsec and the chromospheric network on a scale of 29, 44, and 74 arcsecs are determined using autocorrelation spectral analysis. The two data sets are compared using cross-correlation analysis. The results confirm an earlier conclusion concerning the physical relationship between radio granulation and the calcium chromospheric network.

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