Enhancement of the solar X-ray line intensities due to dielectronic recombination as an excitation process-Reference-Cited by-同舟云学术

Enhancement of the solar X-ray line intensities due to dielectronic recombination as an excitation process

Published:1975-03 Issue:1 Volume:41 Page:97-107
ISSN:0038-0938
Container-title:Solar Physics
language:en
Short-container-title:Sol Phys

Author:

Ansari S. M. Razaullah,Alam Badr�

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/BF00152960.pdf

Reference38 articles.

1. Acton, L. W., Catura, R. C., Meyerott, A. J., and Wolfson, C. J.: 1972, Solar Phys. 26, 183.

2. Aldrovandi, S. M. V. and Péquignot, D.: 1973, Astron. Astrophys. 25, 137.

3. Allen, J. W. and Dupree, A. K.: 1969, Astrophys. J. 155, 27.

4. Ansari, S. M. R. and Alam, B.: 1974, in A. K. Asundi and K. D. Abhyankar (eds.); Proceedings of the Symposium on the Spectroscopic Studies of Astrophysical Interest, Osmania University Press, Hyderabad, in press.

5. Ansari, S. M. R., Elwert, G., and Mücklich, P.: 1970, Z. Naturforsch. 25a, 1781.

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