The brightness of the solar disk in the continuum in the region 1.0?2.4 �m-Reference-Cited by-同舟云学术

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The brightness of the solar disk in the continuum in the region 1.0?2.4 �m

Published:1994-06 Issue:1 Volume:152 Page:47-52
ISSN:0038-0938
Container-title:Solar Physics
language:en
Short-container-title:Sol Phys

Author:

Makarova E. A.,Roshchina E. M.,Sarychev A. P.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/BF01473182.pdf

Reference19 articles.

1. Arvesen, J.C., Griffin, R.N., and Pearson, B.D.:1969,Appl. Optics 8, 2215

2. John,T.L.: 1989,Mon. Not. Roy. Astron. Soc. 240, 1.

3. John,T.L.: 1991,Astron. Astrophys. 244, 511.

4. Kourganoff, V.: 1949,Contrib. Inst. Astroph. Paris 228, 2011.

5. Labs, D. and Neckel, H.: 1968,Z.f.Astrophys. 69, 1.

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. Infrared Photometry of Solar Photospheric Structures. II. Center‐to‐Limb Variation of Active Regions;The Astrophysical Journal;2002-05-10

2. Infrared Photometry of Solar Photospheric Structures. I. Active Regions at the Center of the Disk;The Astrophysical Journal;2000-12

3. Infrared photometry of solar active regions;Journal of Astrophysics and Astronomy;2000-09

4. Infrared Photometry of Solar Active Regions;International Astronomical Union Colloquium;2000

5. The solar continuum in the 0.33–2.45 μm range from the results of observation;Astronomical & Astrophysical Transactions;1997-07

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