Solar activity index for long-term ionospheric forecasts
- 作者: Deminov M.G.1
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隶属关系:
- Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation
- 期: 卷 54, 编号 1 (2016)
- 页面: 1-7
- 栏目: Article
- URL: https://journals.rcsi.science/0010-9525/article/view/153309
- DOI: https://doi.org/10.1134/S0010952516010068
- ID: 153309
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详细
Based on the comparison of solar activity indices (annual average values of the relative number of sunspots Rz12 and solar radio emission flux at a wavelength of 10.7 cm F12) with the ionospheric index of solar activity IG12 for 1954–2013, we have found that the index F12 is a more accurate (than Rz12) indicator of solar activity for the long-term forecast of foF2 (the critical frequency of the F2-layer). This advantage of the F12 index becomes especially significant after 2000 if the specific features of extreme ultraviolet radiation of the Sun are additionally taken into account in the minima of solar cycles, using an appropriate correction to F12. Qualitative arguments are given in favor of the use of F12 for the long-term forecast of both foF2 and other ionospheric parameters.
作者简介
M. Deminov
Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation
编辑信件的主要联系方式.
Email: deminov@izmiran.ru
俄罗斯联邦, Moscow, 142190
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