The effects of solar flares on the very low frequency signals recorded by super SID system
- 作者: Canyilmaz M.1, Guzel E.1, Akdogan T.1
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隶属关系:
- Department of Physics, Faculty of Science
- 期: 卷 24, 编号 3 (2016)
- 页面: 232-237
- 栏目: Electromagnetic Waves in the Ionosphere
- URL: https://journals.rcsi.science/1541-308X/article/view/217593
- DOI: https://doi.org/10.3103/S1541308X16030079
- ID: 217593
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详细
Solar flares cause sudden disturbances at the Earth’s ionosphere. These effects are detected by the very low frequency (VLF), 3−30-kHz signals which are propagated at the Earth-ionosphere waveguide. The sudden changes on the time-dependent intensity of VLF signals are recorded by Super SID system during February, March, and April, 2013. Then VLF data were compared with the GOES satellite data found in the Space Environment Center online database. The main factors of the variation in VLF signal intensities recorded by the Super SID system are class, duration of the solar flare and the frequency of VLF signals.
作者简介
M. Canyilmaz
Department of Physics, Faculty of Science
编辑信件的主要联系方式.
Email: mcanyilmaz@firat.edu.tr
土耳其, Elazig, 23169
E. Guzel
Department of Physics, Faculty of Science
Email: mcanyilmaz@firat.edu.tr
土耳其, Elazig, 23169
T. Akdogan
Department of Physics, Faculty of Science
Email: mcanyilmaz@firat.edu.tr
土耳其, Elazig, 23169
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