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Gloeckler, G.; Hovestadt, D.; Klecker, B.; Vollmer, O.; Fan, C.Y.
Maryland Univ., College Park (USA). Dept. of Physics and Astronomy1975
Maryland Univ., College Park (USA). Dept. of Physics and Astronomy1975
AbstractAbstract
[en] An unusual spectral feature and anomalously large abundance of helium between 0.6 and approximately 2 MeV per nucleon observed during the most quiet time periods in 1974 and 1975 indicate the presence of low-energy helium of an unknown origin. Alphas below 0.6 MeV per nucleon and protons below 1.5 MeV have an E to the minus 1.8 power spectrum, and the proton to alpha ratio is about 30. These particles, of 1 MeV or less, are found to be emitted continuously by the Sun, even during its most inactive periods
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Aug 1975; 23 p; NASA-CR--145861; TR--76-023; Available from NTIS. $3.50.
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