Origin of the weakening of EUV emission lines formed in the chromosphere-corona transition zone-Reference-Cited by-同舟云学术

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Origin of the weakening of EUV emission lines formed in the chromosphere-corona transition zone

Published:1983-05 Issue:1 Volume:85 Page:65-82
ISSN:0038-0938
Container-title:Solar Physics
language:en
Short-container-title:Sol Phys

Author:

Nishikawa Takara

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/BF00148258.pdf

Reference56 articles.

1. Athay, R. G.: 1976, The Solar Chromosphere and Corona: Quiet Sun, D. Reidel Publ. Co., Dordrecht, Holland.

2. Basri, G. S., Linsky, J. L., Bartoe, J.-D. F., Brueckner, G. E., and VanHoosier, M. E.: 1979, Astrophys. J. 230, 924.

3. Beckers, J. M.: 1972, Ann. Rev. Astron. Astrophys. 10, 73.

4. Bonnet, R. M.: 1978, Space Sci. Rev. 21, 379.

5. Bonnet, R. M.: 1979, in M. J. Rycroft (ed.), Space Research, Vol. XX, Pergamon Press.

Cited by 5 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. The Lyman-alpha line in various solar features. I - Observations;The Astrophysical Journal;1988-06

2. Continuum absorption in the solar EUV spectra;Astrophysics and Space Science;1986-01

3. THE QUIET SOLAR TRANSITION REGION;ANNU REV ASTRON ASTR;1986

4. Continuum Absorption in the Solar EUV Spectra;Third Asian-Pacific Regional Meeting of the International Astronomical Union;1986

5. Wavelength-dependence of EUV continuum absorption;Solar Physics;1984-06

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