Density dependence of the line emission of boron-like coronal ions-Reference-Cited by-同舟云学术

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Density dependence of the line emission of boron-like coronal ions

Published:1975-12 Issue:2 Volume:38 Page:369-375
ISSN:0004-640X
Container-title:Astrophysics and Space Science
language:en
Short-container-title:Astrophys Space Sci

Author:

Elwert G.,Raju P. K.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/BF00647137.pdf

Reference10 articles.

1. Austin, W. E., Purcell, T. D., Tousey, R., and Widing, K. G.: 1966,Astrophys. J. 145, 373.

2. Blaha, M.: 1971,Solar Phys. 17, 99.

3. Dankwort, W. and Trefftz, E.: 1974, private communication.

4. Elzner, L.: 1975,Astron. Astrophys., to be published.

5. Garstang, O. H.: 1962,Ann. Astrophys. 25, 109.

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1. Theoretical studies of the atomic transitions in boron-like ions: Mg VIII, Si X and S XII;Journal of Physics B: Atomic, Molecular and Optical Physics;2007-07-25

2. Density and temperature diagnostics of solar emission lines from Navii and Alix;Solar Physics;1994-02

3. EUV spectroscopy as a plasma diagnostic;Space Science Reviews;1993

4. Density measurement from A1 IX ?385.03/?392.42 line ratio;Solar Physics;1991-10

5. OIV and NeVI EUV line ratios in the sun;Advances in Space Research;1991-01

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