An impulsive solar X-ray burst in the energy range 90-400 keV

Details An impulsive solar X-ray burst in the energy range 90-400 keV An impulsive solar X-ray burst in the energy range 90-400 keV

Jun 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975soph...42..441f&link_type=abstract

Solar Physics, vol. 42, June 1975, p. 441-444.

Physics

Solar Flares, Solar Radio Bursts, Solar X-Rays, X Ray Spectra, Balloon-Borne Instruments, H Alpha Line, Solar Spectra, Spectrum Analysis, Time Lag, X Ray Density Measurement

Scientific paper

A hard solar X-ray burst in the energy range 90-400 keV was observed at about 0528:30 UT on 13 April 1974. This event is peculiar in the sense that the X-ray flux is considerably high whereas the corresponding radio and optical flares are of moderate sizes, that the duration of the X-ray burst is very short, and that the X-ray peak is delayed by about 2.5 min relative to the first radio peak.

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