broadbandradiospectralobservationsofthesolareclipseon20080801anditsimplicationsonthequietsunatmosphericmodel | |
TAN BaoLin; YAN YiHua; ZHANG Yin; TAN ChengMin; HUANG Jing; LIU YuYing; FU QiJun; CHEN ZhiJun; LIU Fei; CHEN LinJie | |
刊名 | scienceinchinaseriesgphysicsmechanicsastronomy |
2009 | |
卷号 | 52期号:11页码:1765 |
ISSN号 | 1672-1799 |
英文摘要 | Based on the joint-observations of the radio broadband spectral emissions of the solar eclipse on August 1, 2008 at Jiuquan (total eclipse) and Hualrou (partial eclipse) at the frequencies of 2.00-5.60 GHz (Jiuquan), 2.60-3.80 GHz (Chinese solar broadband radiospectrometer, SBRS/Hualrou), and 5.20-7.60 GHz (SBRS/Hualrou), the authors assemble a successive series of broadband spectra with a frequency of 2.60-7.60 GHz to observe the solar eclipse synchronously. This is the first attempt to analyze the solar eclipse radio emission under the two telescopes located at different places with broadband frequencies in the periods of total and partial eclipses. With these analyses, the authors made a semiempirical model of the coronal plasma density of the quiet Sun, which can be expressed as n(e) similar or equal to 1.42 x 10(9)(r(-2)+1.93r(-5)) (cm(-3)), in the space range of r=1.039-1.212 R-circle dot, and made a comparison with the classic model. |
语种 | 英语 |
内容类型 | 期刊论文 |
源URL | [http://ir.bao.ac.cn/handle/114a11/39421] |
专题 | 中国科学院国家天文台 |
作者单位 | 中国科学院国家天文台 |
推荐引用方式 GB/T 7714 | TAN BaoLin,YAN YiHua,ZHANG Yin,et al. broadbandradiospectralobservationsofthesolareclipseon20080801anditsimplicationsonthequietsunatmosphericmodel[J]. scienceinchinaseriesgphysicsmechanicsastronomy,2009,52(11):1765. |
APA | TAN BaoLin.,YAN YiHua.,ZHANG Yin.,TAN ChengMin.,HUANG Jing.,...&JI GuoShu.(2009).broadbandradiospectralobservationsofthesolareclipseon20080801anditsimplicationsonthequietsunatmosphericmodel.scienceinchinaseriesgphysicsmechanicsastronomy,52(11),1765. |
MLA | TAN BaoLin,et al."broadbandradiospectralobservationsofthesolareclipseon20080801anditsimplicationsonthequietsunatmosphericmodel".scienceinchinaseriesgphysicsmechanicsastronomy 52.11(2009):1765. |
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