Astronomy and Astrophysics – Astronomy
Scientific paper
Jan 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994stin...9622821y&link_type=abstract
Conference Paper, Crimean Astrophysical Observatory USSR
Astronomy and Astrophysics
Astronomy
Radio Observation, Solar Eclipses, Noise Storms, Radio Emission, Radio Astronomy, Radio Sources (Astronomy), Brightness, Accuracy, Universal Time, Very High Frequencies, Solar Diameter
Scientific paper
A method which leads to an increase of accuracy in radio source position and dimension is presented and applied. The radioemission of the solar active regions in the metric band is characterized by a strong and high variability, from which, in this case it is difficult to separate the variations due to the successive occultation of the local sources from the proper variations of the emitting source. It is therefore convenient to count with observations from two observing points, in such a way, that the variations produced by the local sources occultation results from the difference between the radioemission levels in those observing points.
Alvarez O. A.
Rodriguez Rubi E.
Yurovskii Yu.
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