High resolution observations of solar Type-I sources at 460 MHz

Details High resolution observations of solar Type-I sources at 460 MHz High resolution observations of solar Type-I sources at 460 MHz

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984acaps...4....6l&link_type=abstract

(Acta Astrophysica Sinica, vol. 4, no. 1, 3, 1984, p. 6-13) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 8, Sept. 1

Astronomy and Astrophysics

Astrophysics

Noise Storms, Solar Corona, Solar Radio Bursts, Solar Storms, Sunspots, Centimeter Waves, High Resolution, Interferometry, Solar Activity, Solar Limb

Scientific paper

A further, high-resolution study of Type-I sources using the Miyun Compound Interferometer is presented. Type-I sources are divided into 5 morphological classes, multiple-center, single with sharp edges, single with blurred edges, double-component and sources without continuum. Following analyses of the center-limb distribution for the different classes and of source counts according to peak separation for the multiple-center sources, it is ascertained that the cm wave Type-I sources are essentially multiple. The differences between the meter wave and cm wave sources are discussed.

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