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The high-altitude polar wind: Simulation and observation.

机译:高空极风:模拟和观测。

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摘要

In comparing the transport and semikinetic descriptions of the expansion of the polar wind, it is found that the transport model produces shocks in the profiles of all moments, while a generalized semikinetic (GSK) model produces smooth profiles. The inadequacy of the transport model to deal with velocity dispersion, phase mixing and multiple-streams is clearly demonstrated. In the study of the effects of hot magnetospheric electrons on polar outflow, it is found that by imposing a large increase in electron temperature (T{dollar}sb{lcub}rm e{rcub}{dollar}) over a short altitude range, a potential barrier is formed at which H{dollar}sp+{dollar} is partially reflected. For cases in which the T{dollar}sb{lcub}rm e{rcub}{dollar} profile is established by thermal conduction from a high upper boundary T{dollar}sb{lcub}rm e{rcub}{dollar}, the upward flux of H{dollar}sp+{dollar} decreases with increasing upper boundary T{dollar}sb{lcub}rm e{rcub}{dollar}, while O{dollar}sp+{dollar} shows a peak in the upward flux. The polar cap O{dollar}sp+{dollar} data collected by the DE1/RIMS are analyzed by fitting drifting Maxwellian distributions to the retarding potential curves, so that the O{dollar}sp+{dollar} characteristics in terms of its density, velocity and temperature are determined. The results show that these observed data can be matched by the GSK model which includes the effect of centrifugal acceleration due to E {dollar}times{dollar} B convection. The model results also match other observed low- and mid-altitude polar wind density profiles. The matching with satellite data is obtained by using the GSK model which uses observed low-altitude O{dollar}sp+{dollar} polar wind data as lower boundary conditions. Model polar wind density profiles that match mid-altitude satellite data, as well as the newly analyzed O{dollar}sp+{dollar} velocity and temperature, can be obtained when an electron temperature and base ion temperature of 9000 K and an ionospheric convection electric field of 70 mV/m are assumed.
机译:在比较极风膨胀的输运和半动力学描述时,发现输运模型会在所有时刻的轮廓上产生冲击,而广义半动力学(GSK)模型会产生平滑轮廓。清楚地表明了运输模型不足以处理速度分散,相混合和多流。在研究高温磁层电子对极性流出的影响时,发现通过在短高度范围内强加电子温度(T {dollar} sb {lcub} rm e {rcub} {dollar),形成势垒,在该势垒处部分反映H {dol} sp + {dollar}。对于通过高上限T {dollar} sb {lcub} rm e {rcub} {dollar}的热传导建立T {dollar} sb {lcub} rm e {rcub} {dollar}轮廓的情况, H {dollar} sp + {dollar}的向上通量随着上边界T {dollar} sb {lcub} rm e {rcub} {dollar}的增加而减小,而O {dollar} sp + {dollar}则显示出向上通量的峰值。通过将漂移的麦克斯韦分布与延迟势曲线拟合来分析由DE1 / RIMS收集的极极帽O {dollar} sp + {dollar}数据,从而使O {dollar} sp + {dollar}特性在密度,速度方面都具有优势和温度确定。结果表明,这些观测数据可以通过GSK模型进行匹配,该模型包括E {美元} B {对流}对流对离心加速度的影响。模型结果还与其他观测到的低海拔和中海拔极地风密度分布图相匹配。通过使用GSK模型获得与卫星数据的匹配,该模型使用观测到的低空Ospdol + Polar极风数据作为下边界条件。当电子温度和基本离子温度为9000 K且电离层对流电为零时,可以获得与中海拔卫星数据相匹配的模型极风密度剖面,以及新分析的O {dollar} sp + {dollar}速度和温度,假定场强为70 mV / m。

著录项

  • 作者

    Ho, Chi Wing.;

  • 作者单位

    The University of Alabama in Huntsville.;

  • 授予单位 The University of Alabama in Huntsville.;
  • 学科 Physics Fluid and Plasma.; Physics Atmospheric Science.
  • 学位 Ph.D.
  • 年度 1993
  • 页码 226 p.
  • 总页数 226
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 等离子体物理学;大气科学(气象学);
  • 关键词

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