Radar scattering by anisotropic Langmuir turbulence

作者: V.N. Mel'nik

DOI: 10.1023/A:1005048521041

关键词:

摘要: Radar scattering by anisotropic Langmuir turbulence generated Type III electrons is discussed. It shown that in the framework of this model effective echo cross sections, altitudes, and bandwidths profiles can be understood.

参考文章(4)
D. G. Wentzel, A new interpretation of James's solar radar echoes involving lower-hybrid waves The Astrophysical Journal. ,vol. 248, pp. 1132- ,(1981) , 10.1086/159242
I. V. Chashei, V. I. Shishov, Volume scattering model for interpretation of solar radar experiments Solar Physics. ,vol. 149, pp. 413- 416 ,(1994) , 10.1007/BF00690627
Jesse C. James, Radar Studies of the Sun at 38 Mc/s The Astrophysical Journal. ,vol. 146, pp. 356- ,(1966) , 10.1086/148899