A comparison of positions and sizes of sources of centimeter and X-ray bursts

Details A comparison of positions and sizes of sources of centimeter and X-ray bursts A comparison of positions and sizes of sources of centimeter and X-ray bursts

Dec 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976soph...50..429k&link_type=abstract

Solar Physics, vol. 50, Nov.-Dec. 1976, p. 429-436.

Astronomy and Astrophysics

Astronomy

11

Solar Flares, Solar Radio Bursts, Solar X-Rays, Spaceborne Astronomy, Correlation, H Alpha Line, Microwave Interferometers, Skylab Program, Solar Spectra, Time Dependence, X Ray Sources

Scientific paper

Results are reported for a parallel study of three centimeter-wave radio bursts observed on August 9, 1973, with the NRAO three-element interferometer at 3.7 and 11.1 cm and the associated X-ray flares observed with the S-054 telescope aboard Skylab. Within the errors of the measurements, the radio and X-ray events are cospatial. Good agreement is found between the size of the X-ray kernel and that of the core of the centimeter burst, but there is evidence that much of the impulsive radio flux was produced in a larger area.

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