Excitation equilibrium for low lying levels in Cii, Niii, Oiv, Nevi, Mgviii, Six, and Siii-Reference-Cited by-同舟云学术

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Excitation equilibrium for low lying levels in Cii, Niii, Oiv, Nevi, Mgviii, Six, and Siii

Published:1978-07 Issue:2 Volume:58 Page:291-297
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/BF00157274.pdf

Reference16 articles.

1. Ansari, S. M. R. and Alam, B.: 1975, Solar Phys. 41, 97.

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

3. Blaha, M.: 1968, Ann. Astrophys. 31, 311.

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

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

Cited by 7 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Density dependence of solar emission lines of Si(X) and S(XII);Journal of Quantitative Spectroscopy and Radiative Transfer;1983-12

2. Intensity of lines from low-lying levels in C ii, N iii, O iv, Ne vi, Mg viii, Si x, and Si ii;Solar Physics;1982-01

3. Effect of dielectronic recombination excitation in the solar chromosphere-corona transition region;Journal of Quantitative Spectroscopy and Radiative Transfer;1981-08

4. Intensity of astrophysical lines in the transition region;Physica B+C;1981-07

5. Effect of dielectronic recombination excitation on solar line intensities;Journal of Quantitative Spectroscopy and Radiative Transfer;1980-06

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