首页> 外文期刊>Journal of atmospheric and solar-terrestrial physics >Correlations between ULF wave power, solar wind speed, and relativistic electron flux in the magnetosphere: solar cycle dependence
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Correlations between ULF wave power, solar wind speed, and relativistic electron flux in the magnetosphere: solar cycle dependence

机译:ULF波功率,太阳风速和磁层相对论电子通量之间的相关性:太阳周期依赖性

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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 (v_(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 vSW 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 v_(SW) in driving a given ULF power response is solar cycle dependent. Peak ULF power and peak ROCC (~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 v_(SW) and ULF power with MeV electron flux, these correlations being more strongly dependent on solar cycle phase. The v_(SW) 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 ~2 days), before subsequently peaking at lower L-shells. Importantly, our results indicate that v_(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.
机译:我们提供了基于地面相关的1-10 mHz超低频(ULF)波功率,上游太阳风速(v_(SW))和跨外部辐射的MeV电子通量之间的秩相关系数(ROCC)分析的结果带。我们使用了来自SAMNET和IMAGE阵列的地磁仪的完整太阳周期(1990-2001年)数据,以及来自地球同步轨道(GEO)的洛斯阿拉莫斯航天器以及来自L = 5.5和4.5的HEO航天器的MeV电子数据。我们发现在所有本地时间以及L = 3.1到6.6之间的所有L壳层上,ULF波功率与vSW之间都具有非常高的相关性。尽管在驱动给定的ULF功率响应中v_(SW)的效率与太阳周期有关,但在整个太阳周期中仍保持了非常强的L型壳ULF功率相干性。在1994-1995年左右的太阳周期下降阶段,观测到了ULF峰值功率和ROCC峰值(〜0.75),在2000年接近太阳能最大值的较慢平均vSW条件下,这些参数出现了较小的局部峰值。 v_(SW)和ULF功率与MeV电子通量的相关性,这些相关性更强烈地依赖于太阳周期相位。当辐射带最强烈时,v_(SW)和ULF功率与MeV电子通量峰值在太阳周期的后期下降阶段相关。我们的结果证实,辐射带通量在整个太阳周期内都表现出极强的整体L型壳跨相干性。 vSW或ULF功率与MeV电子通量之间的ROCC表现出跟随vSW或ULF功率峰值之后的清晰而系统的时滞。电子通量首先在GEO(滞后〜2天)响应,然后在较低的L壳层达到峰值。重要的是,我们的结果表明,与v_(SW)相关的MeV电子加速过程通过向内径向传输进行操作。 ULF功率与MeV能量电子通量之间的相关性进一步表明,通过ULF波增强的径向扩散,ULF波可能是因果关系。

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