Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mmsai..55..251a&link_type=abstract
(European Physical Society, Ministero della Pubblica Istruzione, and Universita di Catania, EPS Study Conference on Oscillations
Astronomy and Astrophysics
Astronomy
Brightness Temperature, Solar Eclipses, Solar Oscillations, Solar Radio Emission, Dicke Radiometers, Microwave Spectra, Power Spectra, Solar Flux Density, Solar Spectra, Spectrum Analysis
Scientific paper
Changes in solar radio brightness temperature were derived at 2.8, 19.3 and 22.2 GHz from the observations of solar radio flux during the total eclipse on February 16, 1980. High resolution MEM spectra of the brightness temperature fluctuations at the three frequencies showed periodicities ranging from 3.5 min to 128 min. Between 3.5 min and 14.6 min there are a number of comparable significant periodicities common to the three operating frequencies. These periodic variations in brightness temperature may be a result of the spatial and/or temporal variations in the solar radio emissions. Under the assumption of spatial variation, the observed periodicities imply scale sizes of radio emission regions in the range 70,000 km to 600,000 km. Results of the spectral analysis of brightness temperature fluctuations derived from the total solar eclipse observations at 2.8 GHz were reported earlier (Alurkar et al., 1983). In this paper the results of similar analysis for 19.3 and 22.2 GHz are presented and compared with earlier results.
Alurkar Sadanand K.
Bhonsle Rajaram V.
Calla P. N. O.
Degaonkar S. S.
Raju G.
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