Correlations between ULF wave power, solar wind speed, and relativistic electron flux in the magnetosphere: solar cycle dependence

被引:93
作者
Mann, IR [1 ]
O'Brien, TP
Milling, DK
机构
[1] Univ Alberta, Dept Phys, Edmonton, AB T6G 2J1, Canada
[2] Univ York, Dept Phys, York YO10 5DD, N Yorkshire, England
[3] Aerosp Corp, Dept Space Sci, Los Angeles, CA 90009 USA
基金
美国国家航空航天局;
关键词
outer radiation belt dynamics; ULF pulsations; solar-terrestrial coupling; space weather;
D O I
10.1016/j.jastp.2003.10.002
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
We present results from a rank order correlation coefficient (ROCC) analysis between ground-based 1-10 mHz ultra-low frequency (ULF) wave power, upstream solar wind speed (u(SW)), and MeV electron flux across the outer radiation belt. We use data spanning a complete solar cycle (1990-2001) from ground magnetometers from the SAMNET and IMAGE arrays, and MeV electron data from the Los Alamos spacecraft at geosynchronous orbit (GEO) and from a HEO spacecraft at L = 5.5 and 4.5. We find a very high correlation between ULF wave power and u(SW) at all local times and on all L-shells between L = 3.1 and 6.6. Very strong cross-L-shell ULF power coherence is maintained throughout the solar cycle, although the efficiency of vsw in driving a given ULF power response is solar cycle dependent. Peak ULF power and peak ROCC ( similar to 0.75) are observed during the declining phase of the solar cycle around 1994-1995, with smaller localised peaks in these parameters occurring during slower average vsw conditions close to solar maximum in 2000. There is also a strong correlation of both vsw and ULF power with MeV electron flux, these correlations being more strongly dependent on solar cycle phase. The vsw and ULF power correlations with MeV electron flux peak during the late declining phase of the solar cycle, when the radiation belts are most intense. Our results confirm that radiation belt flux demonstrates extremely strong global cross-L-shell coherence throughout the solar cycle. The ROCC between vsw or ULF power and MeV electron flux demonstrate a clear and systematic time lag following the peak in either vsw or ULF power. Electron fluxes respond first at GEO (lag similar to 2 days), before subsequently peaking at lower L-shells. Importantly, our results indicate that u(SW)-correlated MeV electron acceleration processes operate by inwards radial transport. The correlation between ULF power and MeV energy electron flux further suggests that ULF waves could be causally responsible via ULF wave enhanced radial diffusion. (C) 2003 Elsevier Ltd. All rights reserved.
引用
收藏
页码:187 / 198
页数:12
相关论文
共 42 条
[1]   LINEAR PREDICTION FILTER ANALYSIS OF RELATIVISTIC ELECTRON PROPERTIES AT 6.6 RE [J].
BAKER, DN ;
MCPHERRON, RL ;
CAYTON, TE ;
KLEBESADEL, RW .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1990, 95 (A9) :15133-15140
[2]   A strong CME-related magnetic cloud interaction with the Earth's magnetosphere: ISTP observations of rapid relativistic electron acceleration on May 15, 1997 [J].
Baker, DN ;
Pulkkinen, TI ;
Li, X ;
Kanekal, SG ;
Ogilvie, KW ;
Lepping, RP ;
Blake, JB ;
Callis, LB ;
Rostoker, G ;
Singer, HJ ;
Reeves, GD .
GEOPHYSICAL RESEARCH LETTERS, 1998, 25 (15) :2975-2978
[3]   Coronal mass ejections, magnetic clouds, and relativistic magnetospheric electron events: ISTP [J].
Baker, DN ;
Pulkkinen, TI ;
Li, X ;
Kanekal, SG ;
Blake, JB ;
Selesnick, RS ;
Henderson, MG ;
Reeves, GD ;
Spence, HE ;
Rostoker, G .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1998, 103 (A8) :17279-17291
[4]   Recurrent geomagnetic storms and relativistic electron enhancements in the outer magnetosphere: ISTP coordinated measurements [J].
Baker, DN ;
Li, X ;
Turner, N ;
Allen, JH ;
Bargatze, LF ;
Blake, JB ;
Sheldon, RB ;
Spence, HE ;
Belian, RD ;
Reeves, GD ;
Kanekal, SG ;
Klecker, B ;
Lepping, RP ;
Ogilvie, K ;
Mewaldt, RA ;
Onsager, T ;
Singer, HJ ;
Rostoker, G .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1997, 102 (A7) :14141-14148
[5]  
Baker R.G., 1986, Journal of Quaternary Science, V1, P91, DOI 10.1002/jqs.3390010202
[6]   Correlation of changes in the outer-zone relativistic-electron population with upstream solar wind and magnetic field measurements [J].
Blake, JB ;
Baker, DN ;
Turner, N ;
Ogilvie, KW ;
Lepping, RP .
GEOPHYSICAL RESEARCH LETTERS, 1997, 24 (08) :927-929
[7]   Acceleration of relativistic electrons via drift-resonant interaction with toroidal-mode Pc5 ULF oscillations [J].
Elkington, SR ;
Hudson, MK ;
Chan, AA .
GEOPHYSICAL RESEARCH LETTERS, 1999, 26 (21) :3273-3276
[8]  
ELKINGTON SR, 2003, J GEOPHYS RES, V108, DOI DOI 10.1029/20014A009202
[9]   The dependence of high-latitude Pc5 wave power on solar wind velocity and on the phase of high-speed solar wind streams [J].
Engebretson, M ;
Glassmeier, KH ;
Stellmacher, M ;
Hughes, WJ ;
Luhr, H .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1998, 103 (A11) :26271-26283
[10]   Relativistic electron dynamics in the inner magnetosphere - a review [J].
Friedel, RHW ;
Reeves, GD ;
Obara, T .
JOURNAL OF ATMOSPHERIC AND SOLAR-TERRESTRIAL PHYSICS, 2002, 64 (02) :265-282