Advances in Space VLF Type Ⅱ Solar Radio Bursts

GAO Guannan1,2,3, WANG Min1,2,3, DONG Liang1,2,3, GUO Shaojie1,2,3

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Journal of Deep Space Exploration ›› 2021, Vol. 8 ›› Issue (4) : 423-432. DOI: 10.15982/j.issn.2096-9287.2020.20190222001
Article
Article

Advances in Space VLF Type Ⅱ Solar Radio Bursts

  • GAO Guannan1,2,3, WANG Min1,2,3, DONG Liang1,2,3, GUO Shaojie1,2,3
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Abstract

Solar flares and coronal mass ejections(CMEs)are the source disturbances of space weather. The type Ⅱ solar radio burst is the result of electromagnetic radiation caused by CME driven shock moving in corona and interplanetary space. Based on the study of solar physics and space weather forecast,the spectrum characteristics and physical causes of type Ⅱ radio burst,especially VLF type Ⅱ solar radio burst,are analyzed,it shows that VLF type Ⅱ solar radio burst can not only be used to estimate the velocity of CME shock,diagnose the coronal magnetic field,but also provide reference for space weather forecast. The research results can provide useful reference for the scientific research of space VLF radio observation equipment.

Keywords

solar eruptions / flare / CME / solar radio bursts

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GAO Guannan, WANG Min, DONG Liang, GUO Shaojie. Advances in Space VLF Type Ⅱ Solar Radio Bursts. Journal of Deep Space Exploration, 2021, 8(4): 423‒432 https://doi.org/10.15982/j.issn.2096-9287.2020.20190222001

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