Abstract

Occurence of a prominent peak in the ion energy spectrum at energies of 0.1 to 0.7 MeV is observed by the IMP‐8 spacecraft during an energetic particle burst in a plasma “dropout” interval at about 37 Re in the earth’s magnetotail. This unusual characteristic in the spectrum is detected for about 2 minutes. By fitting the observed ion spectra to a drifting Kappa distribution, it is found that the ion population can be described as a hot beam with number densities 4 × 10−7 to 5 × 10−4 cm−3 and temperatures 15 to 45 keV, jetting tailward at speeds of 3500 to 7000 km/s. The energy flux density associated with the beam can be as high as 8 × 10−2 ergs cm−2 sec−1.

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