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首页> 外文期刊>Journal of Geophysical Research, A. Space Physics: JGR >Diffuse auroral scattering by whistler mode chorus waves: Dependence on wave normal angle distribution
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Diffuse auroral scattering by whistler mode chorus waves: Dependence on wave normal angle distribution

机译:扩散极光散射通过惠斯勒模式合唱波:波正常角的依赖分布

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Using the statistical CRRES measurements of the electric field intensities of lower band chorus (LBC) and upper band chorus (UBC) around L = 6 under geomagnetically moderate conditions, we evaluate the variations in modeled magnetic field spectral intensity and the resultant changes in resonant scattering rates of plasma sheet electrons caused by different choices of the wave normal distribution. UBC scattering rates inferredfrom electric field measurements show a common trend of decreasing scattering with increasing peak wave normal angle, θ_m, for the plasma sheet electrons at all resonant pitch angles. This trend is mainly due to the lower power of magnetic field as derived from the electric field measurements for oblique waves. The LBC resonant diffusion inferred from electric field measurements shows a considerable increase in scattering rates with increasing θ_m for ~1 keV electrons at all resonant pitch angles and for 3–30 keV electrons over certain ranges of pitch angles, which is contrary to the decrease in wave magnetic field amplitude and results mainly from the decrease in resonant energy and redistribution of the majority of wave power at large wave normal angles for increased peak wave normal angle. LBC‐induced scattering rates of 3–10 keV electrons decrease with increasing θ_m at low pitch angles, consistent with the decrease in wave magnetic field amplitude when θ_m increases. Our investigation demonstrates that the knowledge of the wave normal distribution of LBC and UBC is essential for an accurate quantification of the net resonant scattering rates and loss timescales of the plasma sheet electrons for an improved global simulation of diffuse auroral precipitation and the evolution of plasma sheet electron pitch angle distribution if only measurements of wave electric field intensityare available. In contrast, the diffuse auroral scattering rates calculated from magnetic field measurements are much less sensitive to the assumption on wave normal angle distribution. While UBC scattering with constant magnetic field power is roughly insensitive to the assumed wave normal distribution, LBC scattering with constant magnetic field power becomes more dependent on the assumed wave normal angle distribution, especially for ~1 keV electrons.
机译:使用的统计crr测量电场强度较低的乐队合唱(LBC)和上层乐队合唱团(哥伦比亚大学)在L = 6眼睛温和的条件下,我们评估模拟磁场的变化光谱强度和结果的变化等离子体的共振散射率表电子波的不同选择造成的正态分布。inferredfrom电场测量显示常见的趋势减少散射增加高峰波正常角θ_m,等离子体单电子的共振角度。磁场的力量来源于斜波的电场测量。从电动LBC共振扩散推断实地测量显示了相当大的增加在散射率随着θ_m ~ 1凯文电子共振俯仰角度和对于3-30 keV电子在一定范围内俯仰角度,相反减少在磁场波振幅和结果主要从共振能量和减少多数的波浪发电的再分配大的波正常角度增加峰波正常的角。3 - 10 keV电子减少随着θ_m在低角度,符合减少在波磁场幅值θ_m增加。波的知识正态分布的LBC和哥伦比亚大学是一个准确的必要条件量化的共振散射利率和等离子体的损失时间尺度表全球模拟电子的一种改进扩散极光降水和演变等离子体电子螺旋角分布如果波电场的测量intensityare可用。极光从磁散射率计算实地测量不太敏感假设在正常波角分布。而哥伦比亚大学散射与恒定磁场权力是约对假定的波正态分布,LBC散射常数磁场的力量变得更加依赖假设波正常的角分布,尤其是对~ 1 keV电子。

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