GSTDTAP  > 气候变化
DOI10.1029/2020GL090426
Low frequency radio observations of the ‘quiet’ corona during the descending phase of sunspot cycle 24
R. Ramesh; A. Kumari; C. Kathiravan; D. Ketaki; M. Rajesh; M. Vrunda
2020-09-09
发表期刊Geophysical Research Letters
出版年2020
英文摘要

We carried out a statistical study of the `quiet' solar corona during the descending phase of the sunspot cycle 24 (i.e. 2015 January ‐ 2019 May) using data obtained with the Gauribidanur RAdioheliograPH (GRAPH) at 53 MHz and 80 MHz simultaneously. Our results show that the equatorial (east‐west) diameters of the solar corona at the above two frequencies shrunk steadily. The decrease was found to be due to a gradual reduction in the coronal electron density (Ne). Independent estimates of Ne in the equatorial region of the `background' corona using white‐light coronagraph observations indicate a decline consistent with our findings.

领域气候变化
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文献类型期刊论文
条目标识符http://119.78.100.173/C666/handle/2XK7JSWQ/294002
专题气候变化
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R. Ramesh,A. Kumari,C. Kathiravan,等. Low frequency radio observations of the ‘quiet’ corona during the descending phase of sunspot cycle 24[J]. Geophysical Research Letters,2020.
APA R. Ramesh,A. Kumari,C. Kathiravan,D. Ketaki,M. Rajesh,&M. Vrunda.(2020).Low frequency radio observations of the ‘quiet’ corona during the descending phase of sunspot cycle 24.Geophysical Research Letters.
MLA R. Ramesh,et al."Low frequency radio observations of the ‘quiet’ corona during the descending phase of sunspot cycle 24".Geophysical Research Letters (2020).
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