Artificial Radiation Observed with Ginga Satellite
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概要
- 論文の詳細を見る
The X-ray astronomy satellite Ginga detected radiation of artificial origin with the Gamma-ray Burst Detector (GBD). The transient events of non-cosmic origin appeared in February 1987 when the GBD observations started, and disappeared in June 1988. The typical event consists of the two successive bursts separated by a few min. The burst pair has approximate reflection symmetry; the first burst has a slow rise and a rapid decay, the second has a rapid rise and a slow decay. The geographical distribution of the events and their spectra revealed that they were due to geomagnetically trapped electrons.
- 宇宙航空研究開発機構の論文
著者
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Fenimore E.
Los Alamos National Laboratory
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MAKINO F.
Institute of Space and Astronautical Science
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MURAKAMI T.
Institute of Space and Astronautical Science
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NISHIMURA J.
Institute of Space and Astronautical Science
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KLEBESADEL R.
Los Alamos National Laboratory
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CONNER J.
Los Alamos National Laboratory
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EVANS W.
Los Alamos National Laboratory
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