Space weather monitoring with a system of ground-based cosmic ray detectors
- 作者: Borog V.V.1, Dmitrieva A.N.1, Mishutina Y.N.1
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隶属关系:
- MEPhI (Moscow Engineering Physics Institute) National Research Nuclear University
- 期: 卷 88, 编号 2 (2024)
- 页面: 302-306
- 栏目: Physics of Cosmic Rays
- URL: https://innoscience.ru/0367-6765/article/view/654767
- DOI: https://doi.org/10.31857/S0367676524020236
- EDN: https://elibrary.ru/RQSPNA
- ID: 654767
如何引用文章
详细
For remote identification of the processes of powerful solar activity in the form of CME directed towards the Earth, a technique of flicker noise spectroscopy has been developed. The results of the analysis of geo-effective events (> G1) are presented according to the data of the international network of neutron monitors and the multidirectional muon hodoscope URAGAN, which indicate the appearance of predictors (with an outstrip of 1–2 days) of the CME approach to the Earthʼs orbit.
全文:

作者简介
V. Borog
MEPhI (Moscow Engineering Physics Institute) National Research Nuclear University
编辑信件的主要联系方式.
Email: vvborog@mephi.ru
俄罗斯联邦, Moscow
A. Dmitrieva
MEPhI (Moscow Engineering Physics Institute) National Research Nuclear University
Email: vvborog@mephi.ru
俄罗斯联邦, Moscow
Yu. Mishutina
MEPhI (Moscow Engineering Physics Institute) National Research Nuclear University
Email: vvborog@mephi.ru
俄罗斯联邦, Moscow
参考
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