Intensity of lines from low-lying levels in C ii, N iii, O iv, Ne vi, Mg viii, Si x, and Si ii-Reference-Cited by-同舟云学术

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Intensity of lines from low-lying levels in C ii, N iii, O iv, Ne vi, Mg viii, Si x, and Si ii

Published:1982-01 Issue:1-2 Volume:75 Page:133-137
ISSN:0038-0938
Container-title:Solar Physics
language:en
Short-container-title:Sol Phys

Author:

Chandra Suresh

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/BF00153466.pdf

Reference13 articles.

1. Bely, O. and Faucher, P.: 1970, Astron. Astrophys. 6, 88.

2. Blaha, M.: 1969, Astron. Astrophys. 1, 42.

3. Chandra, S.: 1978, Solar Phys. 58, 291.

4. Chandra, S.: 1979, Physica 98C, 146.

5. Chandra, S. and Dularey, R.: 1980, J. Quant. Spectrosc. Radiat. Transfer 23, 585.

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1. CLOUDY 90: Numerical Simulation of Plasmas and Their Spectra;Publications of the Astronomical Society of the Pacific;1998-07

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