The characteristics of impulsive solar EUV bursts

Details The characteristics of impulsive solar EUV bursts The characteristics of impulsive solar EUV bursts

Apr 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978soph...57..373e&link_type=abstract

Solar Physics, vol. 57, Apr. 1978, p. 373-383.

Physics

22

Far Ultraviolet Radiation, Solar Activity, Solar Temperature, Spectroheliographs, Apollo Telescope Mount, Atmospheric Temperature, Skylab Program, Solar Atmosphere, Solar Radiation

Scientific paper

This paper examines a number of high-time-resolution intensity-time profiles of EUV impulsive bursts as observed by the EUV spectroheliometer carried aboard the Skylab Apollo Telescope Mount. These bursts are found to be synchronous (to within the instrumental time resolution of 5.5 s) in all wavelengths observed, corresponding to emissions from temperatures ranging from upper-chromospheric to coronal. The distribution with temperature of a suitably defined emission-measure parameter is also examined as a function of time throughout the bursts, and a marked similarity in the shape of this distribution, both between different events and throughout the time history of any particular event, is noted. The significance of these observations for physical processes associated with EUV bursts is briefly discussed.

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