First Type III Solar Radio Bursts of Solar Cycle 25

被引:3
|
作者
Kallunki, Juha [1 ]
McKay, Derek [1 ,2 ,3 ]
Tornikoski, Merja [1 ]
机构
[1] Aalto Univ, Metsahovi Radio Observ, Metsahovintie 114, Kylmala 02540, Finland
[2] Turku Univ, FINCA, Vesilinnantie 5, Turun 20014, Finland
[3] Univ Oulu, Sodankyla Geophys Observ, Tahtelantie 62, Sodankyla 99600, Finland
关键词
Corona; radio emission; Instrumentation and data management; Radio bursts; type III;
D O I
10.1007/s11207-021-01790-9
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The minimum of the previous solar cycle, Solar Cycle 24, occurred in December 2019, which also marked the start of the new Solar Cycle 25. The first radio bursts of the new solar cycle were observed in the spring season 2020. In this work we will present three type III solar bursts which were observed in May and June 2020 at radio frequencies between 18 - 90 MHz. There are two radio observatories in Finland that are capable of doing low-frequency solar radio observations: Aalto University Metsahovi Radio Observatory (MRO) and Kilpisjarvi Atmospheric Imaging Receiver Array (KAIRA) of the Sodankyla Geophysical Observatory, University of Oulu. The instruments of the two institutes have different design and characteristics, and they operate in rather different radio interference environments. We will compare simultaneous observations from these two instruments and we will also discuss the properties of these type III solar bursts.
引用
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页数:10
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