Chorus-Driven Outer Radiation Belt Electron Dynamics at Different L-Shells
ZHANG Sai1,2, XIAO Fu-Liang2**
1Hunan Science and Technology Industrial Vocational and Technical College, Xiangtan 411207 2School of Physics and Electronic Sciences, Changsha University of Science and Technology, Changsha 410004
Chorus-Driven Outer Radiation Belt Electron Dynamics at Different L-Shells
ZHANG Sai1,2, XIAO Fu-Liang2**
1Hunan Science and Technology Industrial Vocational and Technical College, Xiangtan 411207 2School of Physics and Electronic Sciences, Changsha University of Science and Technology, Changsha 410004
摘要Energetic outer radiation belt electron phase space density (PSD) evolution due to interaction with whistler-mode chorus at different L−shells is investigated by solving the diffusion equation including cross diffusion terms. It is found that the difference of diffusion rates for different L−shells occurs primarily at pitch angles 0°–50° and around 90°. In particular, diffusion rates for L=6.5 are found to be 5–10 times larger than that for L=3.5 at these pitch angles. In the presence of cross terms, PSD for ∼ MeV electrons after 24 h decreases by about 25, 12, 10 and 8 times at L=3.5, 4.5, 5.5 and 6.5 near the loss cone, and increases by about 55, 45, 30 and 20 times at larger pitch angles, respectively. After 24 h, the ratios between ∼ MeV electron PSDs from simulations without and with cross diffusion at L=3.5, 4.5, 5.5 and 6.5 are about 350, 600, 800 and 800 near the loss cone, and become 5, 5.5, 6.5 and 8 at pitch angle 90°, respectively. These results demonstrate that neglect of cross diffusion generally results in the overestimate of PSD, and the cross diffusion plays a more significant role in the resonant interaction between chorus waves and outer radiation belt electrons at larger L.
Abstract:Energetic outer radiation belt electron phase space density (PSD) evolution due to interaction with whistler-mode chorus at different L−shells is investigated by solving the diffusion equation including cross diffusion terms. It is found that the difference of diffusion rates for different L−shells occurs primarily at pitch angles 0°–50° and around 90°. In particular, diffusion rates for L=6.5 are found to be 5–10 times larger than that for L=3.5 at these pitch angles. In the presence of cross terms, PSD for ∼ MeV electrons after 24 h decreases by about 25, 12, 10 and 8 times at L=3.5, 4.5, 5.5 and 6.5 near the loss cone, and increases by about 55, 45, 30 and 20 times at larger pitch angles, respectively. After 24 h, the ratios between ∼ MeV electron PSDs from simulations without and with cross diffusion at L=3.5, 4.5, 5.5 and 6.5 are about 350, 600, 800 and 800 near the loss cone, and become 5, 5.5, 6.5 and 8 at pitch angle 90°, respectively. These results demonstrate that neglect of cross diffusion generally results in the overestimate of PSD, and the cross diffusion plays a more significant role in the resonant interaction between chorus waves and outer radiation belt electrons at larger L.
ZHANG Sai;XIAO Fu-Liang**
. Chorus-Driven Outer Radiation Belt Electron Dynamics at Different L-Shells[J]. 中国物理快报, 2010, 27(12): 129401-129401.
ZHANG Sai, XIAO Fu-Liang**
. Chorus-Driven Outer Radiation Belt Electron Dynamics at Different L-Shells. Chin. Phys. Lett., 2010, 27(12): 129401-129401.
[1] Baker D N 2002 Science 297 1486
[2] Summers D, Thorne R M and Xiao F L 1998 J. Geophys. Res. 103 20487
[3] Li L, Cao J and Zhou G 2005 J. Geophys. Res. 110 A03203
[4] Xiao F L and He H Y 2006 Chin. Phys. Lett. 23 267
[5] Xiao F L, Thorne R M and Summers D 2007 Planet. Space Sci 55 1257
[6] Zheng H N, Su Z P and Xiong M 2008 Chin. Phys. Lett. 25 3515
[7] Zong Q G, Zhou X Z, Li X et al 2007 Geophys. Res. Lett. 34 L12105
[8] Zong Q G, Zhou X Z, Wang Y F et al 2009 J. Geophys. Res. 114 A10204
[9] Su Z P, Zheng H N and Wang S 2009 J. Geophys. Res. 114 A07201
[10] Summers D, Ni B and Meredith N P 2007 J. Geophys. Res. 112 A04206
[11] Varotsou A, Boscher D, Bourdarie S, Horne R B, Glauert S A and Meredith N P 2005 Geophys. Res. Lett. 32 L19106
[12] Horne R B, Thorne R M, Glauert S A, Albert J M, Meredith N P and Anderson R R 2005 J. Geophys. Res. 110 A03225
[13] Su Z P, Zheng H N 2008 Chin. Phys. Lett. 25 4493
[14] Li W, Shprits Y Y and Thorne R M 2007 J. Geophys. Res. 112 A10220
[15] Su Z P, Zheng H N and Wang S 2009 J. Geophys. Res. 114 A08202
[16] Shprits Y Y, Thorne R M, Horne R B and Summers D 2009 J. Geophys. Res. 114 A11205
[17] Xiao F L, Su Z P, Zheng H N and Wang S 2009 J. Geophys. Res. 114 A03201
[18] Fok M C, Horne R B, Meredith N P and Glauert S A 2008 J. Geophys. Res. 113 A03S08
[19] Albert J M 2007 J. Geophys. Res. 112 A12202
[20] Tao X, Chan A A, Albert J M and Miller J A 2008 J. Geophys. Res. 113 A07212
[21] Tao X, Albert J M and Chan A A 2008 J. Geophys. Res. 114 A02215
[22] Su Z P, Zheng H N and Xiong M 2009 Chin. Phys. Lett. 26 039401
[23] Xiao F L, Su Z P, Zheng H N and Wang S 2009 J. Geophys. Res. 115 A05216
[24] Glauert S A and Horne R B 2005 J. Geophys. Res. 110 4206
[25] Summers D 2005 J. Geophys. Res. 110 A08213
[26] Meredith N P, Horne R B, Thorne R M and Anderson R R 2003 Geophys. Res. Lett. 30 1871
[27] Albert J M 2003 J. Geophys. Res. 108 1249
[28] Summers D, Ni B and Meredith N P 2007 J. Geophys. Res. 112 A04207
[29] Albert J M and Young S L 2005 Geophys. Res. Lett. 32 14110
[30] Su Z P, Zheng H N and Wang S 2010 J. Geophys. Res. 115 A05219
[31] Su Z P, Zheng H N and Wang S 2010 J. Geophys. Res. 115 A06203
[32] Su Z P, Zheng H N 2009 Chin. Phys. Lett. 26 129401
[33] Su Z P, Xiao F L, Zheng H N and Wang S 2010 J. Geophys. Res. 115 A09208
[34] Reeves G D, K L McAdams, R H W Friedel and T P O' Brien 2003 Geophys. Res. Lett. 30 1529