Observed intensity of the solar continuum over the range 0.33–2.45 μm-Reference-Cited by-同舟云学术

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Observed intensity of the solar continuum over the range 0.33–2.45 μm

Published:1996-10 Issue:10 Volume:39 Page:825-827
ISSN:0033-8443
Container-title:Radiophysics and Quantum Electronics
language:en
Short-container-title:Radiophys Quantum Electron

Author:

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

Publisher

Springer Science and Business Media LLC

Subject

Electrical and Electronic Engineering,Astronomy and Astrophysics,Nuclear and High Energy Physics,Statistical and Nonlinear Physics,Electronic, Optical and Magnetic Materials

Link

http://link.springer.com/content/pdf/10.1007/BF02120965.pdf

Reference17 articles.

1. G. W. Lockwood, H. Tug, and N. M. White,Astrophys. J.,390, 668 (1992).

2. K. A. Burlov-Vasil'yev, É. A. Gurtovenko, and Yu. V. Matveev,Kinem. Fiz. Neb. Tel,10, No. 3, 3 (1994).

3. E. A. Makarova, A. V. Kharitonov, and T. V. Kazachevakaya,Solar Radiant Flux [in Russian], Nauka, Moscow (1991).

4. A. K. Pierce and J. H. Waddel,Mem. R. Astron. Soc.,68, 89 (1961).

5. T. L. John,Mon. Not. R. Astron. Soc.,240, 1 (1989).

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