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The traditional simulation model of sulfur hexafluoride ionosphere release is a simple point-source model and the simulation precision is not high. The three-dimensional refined simulation model of rocket SF6 release is established in this paper, in which the rocket pose and velocity, gas injection velocity and flow, and wind velocity are all taken into account in the diffusion equation. Meanwhile, the influences of geomagnetic inclination and the field diffusion on artificial disturbance form are considered in the plasma diffusion equation, and the two-dimensional plasma diffusion equation is extended to three-dimensional case. The ray tracing method is used to study the influence of ionospheric artificial disturbance on the short wave propagation path. The research results of the ionosphere kinetics process, ionospheric uneven body generation mechanism and evolution are of great significance.
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Keywords:
- ionosphere /
- chemical release /
- sulfur hexafluoride /
- effects
[1] Howard D E, John F B, Edward R M, Cooper C D 1956 J. Geophys. Res. 61 82
[2] Klobuchar J A, Abdu M A 1989 J. Geophys. Res.:Space Phys. 94 2721
[3] Gurnett D A, Anderson R R, Bernhardt P A 1986 J. Geophys. Res. Lett. 13 644
[4] Bernhardt P A, Rousseldupre R A, Pongratz M B 1987 J. Geophys. Res.:Space Phys. 92 5777
[5] Huba J D, Bernhardt P A 1992 J. Geophys. Res.:Space Phys. 97 11
[6] Bernhardt P A, Huba J D 1993 J. Geophys. Res. 98 1613
[7] Wescott E M, Stenbaek-Nielsen H C, Hampton D L 1994 J. Geophys. Res. 99 2145
[8] Bernhardt P A, Baumgardner J B, BhattA N 2011 IEEE Trans. Plasma Sci. 39 2774
[9] Joshi D, Groves K, McNeil W 1997 Modeling the High Frequency Propagation Environment in Metal Oxide Space Cloud Experiment (American:Elsevier Science Inc.) p174
[10] Caton R G, Pederson T R, Parris R T, Groves K M, Bernhardt P A, Cannon P S 2013 American Geophysical Union, Fall Meeting, Moscone, American, December 9-13, 2013#SA21A-2011
[11] Natasha J B, Paul C, Matthew A, Ronald C, Keith G, Todd P, Richard P, Su Y J, et al. 2014 Proceedings of the XXXIst URSI General Assembly and Scientific Symposium Beijing, Chinese, August 17-23, 2014 p1362
[12] Groves K M, Caton R G, Pedersen T R, Parris R T, Su Y J, Cannon P S, Natasha J B, Angling M J, Retterer J M 2013 American Geophysical Union, Fall Meeting Moscone, American, December 9-13, 2013#SA23B-05
[13] Bernhardt P A 1979 J. Geophys. Res. 84 4341
[14] Bernhardt P A 1984 J. Geophys. Res. 89 3929
[15] Bernhardt P A 1979 J. Geophys. Res. 84 793
[16] Bernhardt P A 1982 J. Geophys. Res. 87 7539
[17] Scales W A, Bernhardt P A 1991 J. Geophys. Res. 96 13815
[18] Hu Y G, Zhang Y N, Zhao Z Y 2010 Acta Phys. Sin. 59 8293 (in Chinese)[胡耀垓, 张援农, 赵正予2010 59 8293]
[19] Hu Y G, Zhao Z Y, Zhang Y N 2011 J. Geophys. Res. 116 doi:10.1029/2011JA016438
[20] Huang W G, Gu S F 2006 J. Space Sci. 28 81(in Chinese)[黄文耿, 古士芬2006空间科学学报28 81]
[21] Schunk R W, Szuszczewicz E P 1991 J. Geophys. Res. 96 1337
[22] Gatsonis N A, Hastings D E 1991 J. Geophys. Res. 96 7623
[23] Bernhardt P A 1988 J. Geophys. Res. 93 8696
[24] Bernhardt P A 1987 J. Geophys. Res. 92 4617
[25] Haselgrove J 1955 Proc. Phys. Soc. 23 355
[26] John M K 1968 Radio Sci. l3 1
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[1] Howard D E, John F B, Edward R M, Cooper C D 1956 J. Geophys. Res. 61 82
[2] Klobuchar J A, Abdu M A 1989 J. Geophys. Res.:Space Phys. 94 2721
[3] Gurnett D A, Anderson R R, Bernhardt P A 1986 J. Geophys. Res. Lett. 13 644
[4] Bernhardt P A, Rousseldupre R A, Pongratz M B 1987 J. Geophys. Res.:Space Phys. 92 5777
[5] Huba J D, Bernhardt P A 1992 J. Geophys. Res.:Space Phys. 97 11
[6] Bernhardt P A, Huba J D 1993 J. Geophys. Res. 98 1613
[7] Wescott E M, Stenbaek-Nielsen H C, Hampton D L 1994 J. Geophys. Res. 99 2145
[8] Bernhardt P A, Baumgardner J B, BhattA N 2011 IEEE Trans. Plasma Sci. 39 2774
[9] Joshi D, Groves K, McNeil W 1997 Modeling the High Frequency Propagation Environment in Metal Oxide Space Cloud Experiment (American:Elsevier Science Inc.) p174
[10] Caton R G, Pederson T R, Parris R T, Groves K M, Bernhardt P A, Cannon P S 2013 American Geophysical Union, Fall Meeting, Moscone, American, December 9-13, 2013#SA21A-2011
[11] Natasha J B, Paul C, Matthew A, Ronald C, Keith G, Todd P, Richard P, Su Y J, et al. 2014 Proceedings of the XXXIst URSI General Assembly and Scientific Symposium Beijing, Chinese, August 17-23, 2014 p1362
[12] Groves K M, Caton R G, Pedersen T R, Parris R T, Su Y J, Cannon P S, Natasha J B, Angling M J, Retterer J M 2013 American Geophysical Union, Fall Meeting Moscone, American, December 9-13, 2013#SA23B-05
[13] Bernhardt P A 1979 J. Geophys. Res. 84 4341
[14] Bernhardt P A 1984 J. Geophys. Res. 89 3929
[15] Bernhardt P A 1979 J. Geophys. Res. 84 793
[16] Bernhardt P A 1982 J. Geophys. Res. 87 7539
[17] Scales W A, Bernhardt P A 1991 J. Geophys. Res. 96 13815
[18] Hu Y G, Zhang Y N, Zhao Z Y 2010 Acta Phys. Sin. 59 8293 (in Chinese)[胡耀垓, 张援农, 赵正予2010 59 8293]
[19] Hu Y G, Zhao Z Y, Zhang Y N 2011 J. Geophys. Res. 116 doi:10.1029/2011JA016438
[20] Huang W G, Gu S F 2006 J. Space Sci. 28 81(in Chinese)[黄文耿, 古士芬2006空间科学学报28 81]
[21] Schunk R W, Szuszczewicz E P 1991 J. Geophys. Res. 96 1337
[22] Gatsonis N A, Hastings D E 1991 J. Geophys. Res. 96 7623
[23] Bernhardt P A 1988 J. Geophys. Res. 93 8696
[24] Bernhardt P A 1987 J. Geophys. Res. 92 4617
[25] Haselgrove J 1955 Proc. Phys. Soc. 23 355
[26] John M K 1968 Radio Sci. l3 1
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