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The Charge and Isotopic Composition of Solar Cosmic Rays

Published online by Cambridge University Press:  25 May 2016

Frank B. McDonald*
Affiliation:
NASA Goddard Space Flight Center, Greenbelt, Md., U.S.A.

Abstract

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The charge and isotopic composition of solar cosmic rays potentially contain a wealth of information on the acceleration and confinment of energetic particles at the Sun. As the experimental techniques have improved and with the increasing number of measurements, this potential is now being realized. It is convenient to divide the composition studies into three areas: (a) helium-iron, with energies >10 MeV nuc−1; (b) helium-iron, and the trans-iron elements, with energies <2 MeV nuc−1; (c) the isotopic composition. In the first area at energies above 10 MeV nuc−1 the solar cosmic rays appear to provide a representative sample of the solar corona. At lower energies (b) complex enhancement effects are noted. These increase with Z and decrease with energy. This result as well as the high abundance of 3He suggest that the acceleration process is not a simple one and probably several stages are required.

Type
Part IV Acceleration, Containement and Emission of High-Energy Flare Particles
Copyright
Copyright © Reidel 1974 

References

Anglin, J. D., Dietrich, W. F., and Simpson, J. A.: 1973, in Ramaty, R. and Stone, R. G. (eds.), High Energy Phenomena on the Sun Symposium Proceedings, NASA Goddard Preprint, p. 315.Google Scholar
Armstrong, T. P. and Krimigis, S. M.: 1971, J. Geophys. Res. 76, 4230.CrossRefGoogle Scholar
Bertsch, D. L., Fichtel, C. E., Pellerin, C. J., and Reames, D. V.: 1973, Astrophys. J. 180, 583.Google Scholar
Biswas, S. and Fichtel, C. E.: 1963, Astrophys. J. 139, 941.CrossRefGoogle Scholar
Biswas, S. and Fichtel, C. E.: 1965, Space Sci. Rev. 4, 709–36.CrossRefGoogle Scholar
Biswas, S., Fichtel, C. E., and Guss, D. E.: 1966, J. Geophys. Res. 71, 4071.Google Scholar
Braddy, D., Chan, J., and Price, P. B.: 1973, Phys. Rev. Letters 30, 669.Google Scholar
Crawford, H. J., Price, P. B., and Sullivan, J. D.: 1972, Astrophys. J. 175, L149.Google Scholar
Cartwright, B. G. and Mogro-Campero, A.: 1973, in Ramaty, R. and Stone, R. G. (eds.), High Energy Phenomena on the Sun Symposium Proceedings, NASA Goddard Preprint, p. 393.Google Scholar
Durgaprasad, N., Fichtel, C. E., Guss, D. E., and Reames, D. V.: 1968, Astrophys. J. 154, 307.Google Scholar
Fan, C. Y., Pick, M., Pyle, R., Simpson, J. A., and Smith, D. R.: 1968, J. Geophys. Res. 73, 1555.Google Scholar
Fichtel, C. E. and Guss, D. E.: 1961, Phys. Rev. Letters 6, 495.Google Scholar
Geiss, J.: 1972, in Sonett, C. P., Coleman, P. J., and Wilcox, J. M. (eds.), Proc. Asilomar Conf. on the Solar Wind, NASA, Washington, p. 559.Google Scholar
Gloeckler, G., Fan, C. Y., and Hovestadt, D.: 1973, 13th International Cosmic Ray Conf. Proceedings, University of Denver, 2, p. 1492.Google Scholar
McDonald, F. B. and Desai, U. D.: 1971, J. Geophys. Res. 76, 808.CrossRefGoogle Scholar
McDonald, F. B. and Van Hollebeke, M. A.: 1973, in Ramaty, R. and Stone, R. G. (eds.), High Energy Phenomena on the Sun Symposium Proceedings, NASA Goddard Preprint, p. 404.Google Scholar
Mogro-Campero, A. and Simpson, J. A.: 1972, Astrophys. J. Letters 6, 495.Google Scholar
Price, P. B., Chan, J. H., Crawford, H. J., and Sullivan, J. D.: 1973, 13th International Cosmic Ray Conf. Proceedings, Univ. of Denver, Vol. 2, p. 1479.Google Scholar
Price, P. B. and Chan, J. H.: 1973b, ‘Apollo 17 Preliminary Science Report’, NASA Special Publication, p. 19.Google Scholar
Teegarden, B. J., von Rosenvinge, T. T., and McDonald, F. B.: 1973, Astrophys. J. 180, 571.Google Scholar
Webber, W. R., Roelof, E. C., McDonald, F. B., Teegarden, B. J., and Trainor, J.: 1973, 13th International Cosmic Ray Conf. Proceedings, Vol. 2, p. 1516.Google Scholar