Microwave diagnostics of nonthermal electron characteristics

Chinese Science Bulletin

Volumn 41, Issue 8, 1996, Pages 671-674

  Zhou, Aihua ^a,b   Zhang, Jie ^a   Zhang, Heqi ^a  

^a INSTITUTE OF GEOLOGY AND GEOPHYSICS   (China)

^b CHINESE ACADEMY OF SCIENCES   (China)

Author keywords

Nonthermal electron; Solar microwave burst

Indexed keywords

EID: 0039767008     PISSN: 10016538     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article

References (6)

1. Dulk, G. A., Marsh, K. A., Simplified expressions for the gyrosynchrotron radiation from mildly relativistic nonthermal and thermal electrons, Astrophys. J., 1982, 259: 350.
2. Gary, D., The numbers of fast electrons in solar flares as deduced from hard X-ray and microwave spectral data, Astrophys. J., 1985, 297: 799.
3. Zhou Aihua, The numbers of energetic electrons deduced from a type C microwave burst, Acta Astrophysica Sinica, 1992, 12(2): 148.
4. Wang, H., Gary, D. E., Lim, J., Microwave spectral imaging and hard X-ray observations of a solar limb flare, Astropys. J., 1994, 433: 379.
5. Zhou, A. H., Magnetic field strength estimation in synchrotron radiation sources, Astrophy. and Space Science, 1994, 222: 107.
6. Zhou Ai-hua, Karlicky, M., Magnetic field estimation in microwave radio sources, Solar Phys., 1994, 153: 441.