Abstract
The function and physical mechanism of heat flow and the viscous stress in the velocity distribution function expanded by Maxwellian distribution are presented. With the introduction of effective temperature T f , incoherent scatter spectra from plasma for electromagnetic wave in arbitrary line of sight are given. The effect of asymmetry and anisotropy provided by heat flow and the viscous stress on power spectra is discussed. Radar spectra are calculated for different cases of electric field, direction, collision frequency and temperature. The effect of heat flow and the viscous stress on inversion results is analyzed. With a large electric field, the character of non-Maxwellian must be considered.
Similar content being viewed by others
References
Evans J V. Theory and practice of ionosphere study by Thomson scatter radar. Proc IEEE, 1969, 57(4): 496–530
Raman Venkat R S, St-Maurice J P, Ong R S B. Incoherent scattering of radar waves in the auroral ionosphere. J Geophys Res, 1981, 86(A6): 4751–4762
Zheng C Q, Wu J. A computation of the incoherent radar spectra of non-Maxwellian plasma in the high-latitude ionosphere. Chin J Geophys (in Chinese), 1994, 37(4): 433–439
Wu J. An analytical form of the Raman et al. ion velocity distribution in auroral ionospheric F-region and the distribution saturation with increase of electric field. Chin J Geophys (in Chinese), 1997, 40(1): 739–746
Schunk R W, Walker C G. Ion velocity distributions in the auroral ionosphere. Planet Space Sci, 1972, 20: 2175–2191
St-Maurice J P, Schunk R W. Auroral ion velocity distributions using a relaxation model. Planet Space Sci, 1973, 21: 1115–1130
St-Maurice J P, Schunk R W. Use of generalized orthogonal polynomial solutions of Boltzmann’s equation in certain aeronomy problems: Auroral ion velocity distribution. J Geophys Res, 1976, 81(13): 2145–2154
St-Maurice J P, Schunk R W. Auroral ion velocity distribution for a polarization collision model. Space Sci, 1977, 25: 243–266
St-Maurice J P, Schunk R W. Ion velocity distribution in the high-latitude ionosphere. Rev Geophys Space Phys, 1979, 17(1): 99–134
Hubert D. Auroral ion velocity distribution function: the Boltzmann model revisited. Planet Space Sci, 1982, 30(11): 1137–1146
Hubert D. Auroral ion velocity distribution function: generalized polynomial solution of Boltzmann’s equation. Planet Space Sci, 1983, 31(1): 119–1127
Cooper J, Kohl H. Asymmetric incoherent scatter spectra from a relaxation collision model. J Atoms Terr Phys, 1990, 52: 133–150
Mintzer D. Generalized orthogonal polynomial solutions of the Boltzmann equation. Phys Fluids, 1965, 8(6): 1076–1090
Grad H. Principles of the Kinetic Theory of Gases, Handbuck der Physik XII, 12, Berlin: Springer, 1958. 205–294
Sheffield J. Plasma Scattering of Electromagnetic Radiation, Academic. New York: A subsidiary of Harcourt Brace Jovanovich Publishers, 1975. 113–128
Author information
Authors and Affiliations
Corresponding author
Additional information
Supported by the National Natural Science Foundation of China (Grant No. 40310223)
Rights and permissions
About this article
Cite this article
Xu, B., Xue, K., Wu, J. et al. Incoherent scatter spectra from plasma of a 13-moment approximation distribution function. Sci. China Ser. E-Technol. Sci. 51, 624–631 (2008). https://doi.org/10.1007/s11431-008-0054-4
Received:
Accepted:
Published:
Issue Date:
DOI: https://doi.org/10.1007/s11431-008-0054-4