PMO OpenIR  > 太阳活动的多波段观测研究团组
A method of calculation of the solar radio flux density for high spatial resolution observations
Zhou, SR; Huang, GL
1999
Source PublicationCHINESE PHYSICS LETTERS
ISSN0256-307X
Volume16Issue:3Pages:223-225
AbstractIn this paper we present a method of calculation of the flux density of radio source for high spatial resolution solar radio observations, i.e., according to the observed solar antenna temperature, we make a correction for the K factor of antenna power pattern, then we can obtain values of solar radio flux. According to models of different brightness temperature distributions of the quiet sun and radio sources, we deduced the expression of the K factor of antenna power pattern, and calculated the fluxes of the quiet sun and slowly varying component emission of radio sources at 22 GHz.
Subject AreaPhysics
WOS HeadingsScience & Technology ; Physical Sciences
Indexed BySCI
Language英语
WOS Research AreaPhysics
WOS SubjectPhysics, Multidisciplinary
WOS IDWOS:000079613000024
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Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/8316
Collection太阳活动的多波段观测研究团组
AffiliationChinese Acad Sci, Purple Mt Observ, Nanjing 210008, Peoples R China
Recommended Citation
GB/T 7714
Zhou, SR,Huang, GL. A method of calculation of the solar radio flux density for high spatial resolution observations[J]. CHINESE PHYSICS LETTERS,1999,16(3):223-225.
APA Zhou, SR,&Huang, GL.(1999).A method of calculation of the solar radio flux density for high spatial resolution observations.CHINESE PHYSICS LETTERS,16(3),223-225.
MLA Zhou, SR,et al."A method of calculation of the solar radio flux density for high spatial resolution observations".CHINESE PHYSICS LETTERS 16.3(1999):223-225.
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