The equipment and procedure for observations of dynamic spectra of solar burst emission at the station KRIM
1Yurovsky, YF 1Crimean Astrophysical Observatory, Nauchny, Ukraine |
Kinemat. fiz. nebesnyh tel (Online) 2013, 29(6):68-77 |
Start Page: Instruments and Devices |
Language: Russian |
Abstract: We describe the equipment and procedure for observations of dynamic spectra of solar burst emission at the station KRIM of the Crimean Astrophysical Observatory (CRAO) which is incorporated into the world network e-CALLISTO. The parameters of the antenna made at the Laboratory of Radio Astronomy of the SRI CRAO are described. The method for apparatus distortion exception which is developed at the KRIM station is considered. |
Keywords: KRIM, method, radio emission |
1.G. Z. Aizenberg, Ultrashort Wave Antennae (Svyaz’izdat, Moscow, 1957) [in Russian].
2.N. A. Esepkina, D. V. Korol’kov, and Yu. N. Pariiskii, Radiotelescopes and Radiometers (Nauka, Moscow, 1973) [in Russian].
3.A. D. Kuz’min and A. E. Salomonovich, Radioastronomical Methods for Measuring the Antenna Parameters (Sov. radio, Moscow, 1964) [in Russian].
4.A. O. Benz, C. Monstein, and H. Meyer, “CALLISTO—A new concept for solar radio spectrometers,” Sol. Phys. 226, 143–151 (2005).
https://doi.org/10.1007/s11207-005-5688-9
5.A. O. Benz, C. Monstein, H. Meyer, et al., “A world-wide net of solar radio spectrometers: e-CALLISTO,” Earth, Moon, Planets 104, 277–285 (2009).
https://doi.org/10.1007/s11038-008-9267-6
6.W. C. Erickson, M. R. Kundu, M. J. Mahoney, and T. Gergely, “Dermination of the decameter wavelength spectrum of the quiet Sun,” Solar Phys. 54, 57–63 (1977).
https://doi.org/10.1007/BF00146425
7.Report on the United Nations/European Space Agency/National Aeronautics and Space Administration of the United States of America Workshop on the International Heliophysical Year 2007. http://www.oosa.unvienna.org/pdf/reports/ac105/AC105-856E.pdf