Bremsstrahlung X ray mappings of an intense, widespread, and pulsating electron precipitation event following a sudden commencement

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Bremsstrahlung, Electron Precipitation, Solar Terrestrial Interactions, Spatial Distribution, Sudden Storm Commencements, X Rays, Magnetic Storms, Satellite-Borne Instruments, Spectral Energy Distribution, Temporal Distribution

Scientific paper

For the first time, remote bremsstrahlung X-ray spatial, temporal, and spectral mappings from a satellite are presented for a strong energetic electron precipitation event following a sudden commencement. After the sudden commencement of July 13, 1982, and at the beginning of a magnetospheric substorm, X-rays were observed over a period of more than 4 min from the P78-1 spacecraft at 600-km altitude. The X-rays above 21 keV were emitted over a magnetic local time (MLT) interval spanning 6 hours. Five precipitating temporal spikes were observed with coherency over wide longitude intervals of 3 hours or more in MLT near midnight. The energy spectra over broad longitude intervals tended to be harder simultaneously at the times of greatest X-ray intensity. The power input to the atmosphere from precipitating electrons that produced the X-rays emitted within 220-2230 MLT is estimated to have reached values of 5 x 10 to the 16th ergs/s over an area of about 30,000 sq km, leading to an average energy deposition rate of about 160 ergs/sq cm s. The precipitation inputs at other magnetic local times displayed nearly simultaneous sharp maxima in time but with lower power inputs.

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