电邮这篇文章 Estimation of Solar Activity Based on VHF Radar Data
- 作者: Filippov M.Y.1, Abunin A.A.2,3, Khodataev N.A.1
-
隶属关系:
- 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
- 期: 卷 59, 编号 7 (2019)
- 页面: 950-954
- 栏目: Article
- URL: https://journals.rcsi.science/0016-7932/article/view/157907
- DOI: https://doi.org/10.1134/S0016793219070144
- ID: 157907
如何引用文章
开放存取
##reader.subscriptionAccessGranted##
订阅存取
详细
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.
作者简介
M. Filippov
JSC Mints Moscow Radiotechnical Institute of Russian Academy of Sciences
编辑信件的主要联系方式.
Email: mm.grif@gmail.com
俄罗斯联邦, Moscow, 117519
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
俄罗斯联邦, Troitsk, 142191; Elista, 358000
N. Khodataev
JSC Mints Moscow Radiotechnical Institute of Russian Academy of Sciences
Email: mm.grif@gmail.com
俄罗斯联邦, Moscow, 117519
补充文件
