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Interpretation of solar microwave C type burst spectra in terms of magnetic nonhomogeneity
Yao, JM ; Yu, XF ; Wei, FS
1997
Source PublicationSCIENCE IN CHINA SERIES A-MATHEMATICS PHYSICS ASTRONOMY
ISSN1006-9283
Volume40Issue:12Pages:1325—1330
AbstractThe solar radio spectra of the gyro-synchrotron radiation without absorption from mildly relativistic non-thermal electron have been presented using the model with the spherical symmetric nonhomogeneity. These spectra have the following features: (i) Twists and turns of the spectra, which appear at the joint between the medium and high frequencies. (ii) Flux density drop at the lower frequencies. Even if there are no absorption in the radio sources, flux density drop at the lower frequencies is still present because of magnetic nonhomogeneity. (iii) These theoretical spectra belong to C type. This provides us a new interpretation for the observed solar burst C type spectra.
KeywordSpherical Symmetric Nonhomogeneity Gyrosynchrotron Spectra Twists And Turns Of Spectra Flux Density Drop At Lower Frequencies Solar Radio Burst c Type Spectra
Subject AreaMathematics
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/8412
Collection期刊(老文献)
Recommended Citation
GB/T 7714
Yao, JM,Yu, XF,Wei, FS. Interpretation of solar microwave C type burst spectra in terms of magnetic nonhomogeneity[J]. SCIENCE IN CHINA SERIES A-MATHEMATICS PHYSICS ASTRONOMY,1997,40(12):1325—1330.
APA Yao, JM,Yu, XF,&Wei, FS.(1997).Interpretation of solar microwave C type burst spectra in terms of magnetic nonhomogeneity.SCIENCE IN CHINA SERIES A-MATHEMATICS PHYSICS ASTRONOMY,40(12),1325—1330.
MLA Yao, JM,et al."Interpretation of solar microwave C type burst spectra in terms of magnetic nonhomogeneity".SCIENCE IN CHINA SERIES A-MATHEMATICS PHYSICS ASTRONOMY 40.12(1997):1325—1330.
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