Solar type III bursts with high-frequency cut-off

被引:1
作者
Stanislavsky, A. A. [1 ]
机构
[1] Inst Radio Astron, 4 Mystetstv St, UA-61002 Kharkov, Ukraine
关键词
Sun: corona; Sun: radio radiation; methods: observational; instrumentation: miscellaneous; telescopes; RADIO-BURSTS; DENSITY MODEL; WAVELENGTHS; EMISSION; CORONA;
D O I
10.1002/asna.201613141
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Background: Solar activity often manifests in type III bursts. Some of them can have high-frequency cut-off. The origin of this phenomenon is unclear until now. Materials and Methods: New results in the study of solar bursts with high-frequency cut-off observed with the UTR-2 radio telescope are presented. The bursts were associated with the emergency of a new group of solar spots behind the solar limb relative to an observer on the Earth. Results: We have identified the radio events with type III by analyzing its frequency drift rate, duration and flux depending on frequency. The cut-off feature is considered in the context of specific effects of radio wave propagation between the burst sources moving behind the solar limb and the ground-based radio instruments. Conclusions: The role of tunnel-like cavities with low density in the solar corona can be crucial for the emergence of solar decameter bursts with high-frequency cut-off.
引用
收藏
页码:407 / 412
页数:6
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