Solar X-ray bursts in relation to the microwave bursts and SIDs

Details Solar X-ray bursts in relation to the microwave bursts and SIDs Solar X-ray bursts in relation to the microwave bursts and SIDs

Mar 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975ijrsp...4...24m&link_type=abstract

Indian Journal of Radio and Space Physics, vol. 4, Mar. 1975, p. 24-28.

Astronomy and Astrophysics

Astronomy

H Alpha Line, Microwave Emission, Solar Radio Emission, Solar X-Rays, Sudden Ionospheric Disturbances, Data Correlation, Explorer 37 Satellite, Satellite Observation, Solar Flares, Spaceborne Astronomy

Scientific paper

The paper analyzes different types of X-ray bursts recorded by Explorer 37 in the bands 0.5-3, 1-8, and 8-20 A in relation to their morphological types and peak time attainment, along with their correlations with the microwave bursts of different morphological types, intensity-based classes of H-alpha flares, and different types of sudden ionospheric disturbances (SIDs). X-ray bursts are found to be mainly of three morphological types: impulsive, gradual rise and fall, and gradual rise and quick fall. Impulsive X-ray bursts are mostly associated with bright H-alpha flares as well as with different microwave bursts and SIDs. The peak of X-ray bursts at a shorter wavelength is attained earlier than that at a longer wavelength. A major conclusion is that the simultaneous presence of X-ray and centimeter bursts can only ascertain the subsequent occurrences of SIDs. The percentage correlation of X-ray bursts with SIDs in the presence of microwave bursts is about twice as great as that in the absence of microwave bursts

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