Equator-pole differences in the solar chromosphere from Lyman-continuum data-Reference-Cited by-同舟云学术

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Equator-pole differences in the solar chromosphere from Lyman-continuum data

Published:1972-10 Issue:2 Volume:26 Page:335-342
ISSN:0038-0938
Container-title:Solar Physics
language:en
Short-container-title:Sol Phys

Author:

Vernazza J. E.,Noyes R. W.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/BF00165274.pdf

Reference20 articles.

1. Abetti, G. and Castelli, I.: 1935, Oss. Mem. Arcetri 53, 25.

2. Altrock, R. C. and Canfield, R. C.: 1972, Astrophys. J. 171, L71.

3. Appenzeller, I. and Schröter, E. H.: 1967, Astrophys. J. 147, 1100.

4. Beckers, J. M.: 1960, Bull. Astron. Inst. Neth. 15, 85.

5. Beckers, J. M.: 1968, Solar Phys. 3, 367.

Cited by 3 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. He [CSC]i[/CSC] 10830 Å Wing Asymmetry in Polar Coronal Holes: Evidence for Radial Outflows;The Astrophysical Journal;1996-08-20

2. EUV Observations of the Active Sun from the Harvard Experiment on ATM;Symposium - International Astronomical Union;1975

3. EUV Observations of the Active Sun from the Harvard Experiment on ATM;Solar Gamma-, X-, and EUV Radiation;1975

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