VLF recombination radio lines and a new method of estimating the intensity of soft cosmic rays

Details VLF recombination radio lines and a new method of estimating the intensity of soft cosmic rays VLF recombination radio lines and a new method of estimating the intensity of soft cosmic rays

May 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987pazh...13..191s&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 13, no. 3, 1987, p. 191-198. In Russian. In Russian. In Russian. In

Statistics

Computation

4

Cosmic Rays, Electron Recombination, Line Spectra, Radiant Flux Density, Radio Spectra, Very Low Frequencies, Carbon, Computational Astrophysics, Hydrogen

Scientific paper

Explanations are given for why carbon recombination radio lines are observed at the highest excitation levels in the interstellar medium and why the radio lines of substantially more abundant hydrogen are absent. A new method is proposed for estimating the intensity of soft cosmic rays from the hydrogen-ionization rate measured from the relative intensities of highly excited carbon and hydrogen radio lines. A hydrogen-ionization rate of less than or equal to 1.5 x 10 to the -16th/s toward CasA is obtained.

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