Email this article Estimation of Solar Activity Based on VHF Radar Data
- Authors: Filippov M.Y.1, Abunin A.A.2,3, Khodataev N.A.1
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Affiliations:
- JSC Mints Moscow Radiotechnical Institute of Russian Academy of Sciences
- Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation, Russian Academy of Sciences
- Gorodovikov Kalmyk State University
- Issue: Vol 59, No 7 (2019)
- Pages: 950-954
- Section: Article
- URL: https://journals.rcsi.science/0016-7932/article/view/157907
- DOI: https://doi.org/10.1134/S0016793219070144
- ID: 157907
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Abstract
The index of integral solar activity F10.7 is one of the main input parameters of existing ionospheric models, including the model used at early-warning radar stations to compensate for coordinate information errors; the use of external sources of F10.7 seems to be impossible. A method is presented for highly reliable estimate of the solar X-ray flux values at a wavelength of 10.7 cm based only on the capabilities of the station itself.
About the authors
M. Yu. Filippov
JSC Mints Moscow Radiotechnical Institute of Russian Academy of Sciences
Author for correspondence.
Email: mm.grif@gmail.com
Russian Federation, Moscow, 117519
A. A. Abunin
Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation, Russian Academy of Sciences; Gorodovikov Kalmyk State University
Email: mm.grif@gmail.com
Russian Federation, Troitsk, 142191; Elista, 358000
N. A. Khodataev
JSC Mints Moscow Radiotechnical Institute of Russian Academy of Sciences
Email: mm.grif@gmail.com
Russian Federation, Moscow, 117519
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