Choosing optical materials for diagnostics of the solar atmosphere in the wavelength range of 6

Choosing optical materials for diagnostics of the solar atmosphere in the wavelength range of 6–60 nm

Published:2011-01 Issue:1 Volume:75 Page:84-86
ISSN:1062-8738
Container-title:Bulletin of the Russian Academy of Sciences: Physics
language:en
Short-container-title:Bull. Russ. Acad. Sci. Phys.

Author:

Kuzin S. V.,Polkovnikov V. N.,Salashchenko N. N.

Publisher

Allerton Press

Subject

General Physics and Astronomy

Link

http://link.springer.com/content/pdf/10.3103/S1062873811010151.pdf

Reference4 articles.

1. Oraevskii, V.N., Sobel’man, I.I., Zhitnik, I.A., and Kuznetsov, V.D., Usp. Fiz. Nauk, 2002, vol. 172, p. 949.

2. Braun, St., Dietsch, R., and Haidl, M., Microelectron. Eng., 2001, vols. 57–58, p. 9.

3. Zuev, S.Yu., Kuzin, S.V., Polkovnikov, V.N., and Salashchenko, N.N., Izv. Akad. Nauk. Ser. Fiz., 2010, vol. 74, no. 1, pp. 58–61 [Bull. Russ. Acad. Sci. Phys. (Engl. Transl.), 2010, vol. 74, no. 1, p. 50].

4. Zuev, S.Yu., et al., Materialy XIII Mezhdunar. simpoziuma “Nanofizika i nanoelektronika” (Proc. Int. Symp. “Nanophysics and Nanoelectronics”), Nizhni Novgorod, 2009, p. 62.

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