首页> 外文学位 >INTERPRETING ELECTRON TEMPERATURE CHANGES IN THE LOWER IONOSPHERE.
【24h】

INTERPRETING ELECTRON TEMPERATURE CHANGES IN THE LOWER IONOSPHERE.

机译:下部电离层中解释的电子温度变化。

获取原文
获取原文并翻译 | 示例

摘要

The electron temperature changes due to 3, 5 and 430 MHz radio wave heating in the lower ionosphere are measured using incoherent scatter diagnostic techniques and are also calculated from heating/cooling theory. The experiments were performed at Arecibo Observatory using the new HF heating facility and the Arecibo Observatory 430 MHz incoherent backscatter system. In order to interpret the incoherent scatter results a spectral parameter library is developed which gives the spectral width, the spectral maximum and the bandlimited power of the incoherent scatter spectrum for a wide range of ionospheric parameters.; There are two collisional formulations which have been widely used to reduce incoherent scatter data in the D and E regions: Dougherty and Farley (1963) and Waldteufel (1970). To determine which collisional formulation should be used, we examine the results of recent Arecibo experiments performed in an unheated ionosphere. A comparison of the measured electron-neutral collision frequency values derived from the two different collisional formulations to the predicted model values show excellent agreement for the Dougherty and Farley formulation but less than satisfactory agreement for the Waldteufel formulation.; Using the Dougherty and Farley formulation we determine electron temperature changes from the measured heated-to-ambient spectral parameter ratios. In comparing the measured electron temperature changes to the predicted changes for 430 MHz heating we find a large discrepancy throughout the D and E regions: the measured electron temperature changes are much less than the predicted. The discrepancy in the 75-100 km region can be removed by increasing the model O(,2) rotational cooling rate by a factor of 10, while the discrepancy below 75 km can be removed by a factor of 4 increase. The cooling rate increases, however, are not the only possible explanation for the discrepancies. Two other effects, the non-Maxwellian electron velocity distribution and heat conduction, could remove the discrepancies if the magnitude of their effects were significantly increased in the model. The discrepancies could also be removed by using a f('2.18) frequency scaling law for the predicted heating rather than the currently accepted f('2) law, but there are no physical explanations to support this modification.; The 3 and 5 MHz heating results are in satisfactory agreement with the model if D region absorption is taken into account and, thus, do not support the increased cooling rates suggested by the 430 MHz results. The agreement of these results, however, would not be significantly affected by the other suggested modifications.; The heating due to the 52 (mu)sec diagnostic pulse is also measured. The diagnostic pulse heating at 70 km is found to increase the electron temperature by a factor of 2.85 (+OR-) 1.35 above ambient. Although the error estimates are large, this increase is in agreement with the predictions of the model.
机译:使用非相干散射诊断技术测量下部电离层中由于3、5和430 MHz无线电波加热而引起的电子温度变化,并根据加热/冷却理论计算得出。实验是在Arecibo天文台使用新的HF加热设施和Arecibo天文台430 MHz非相干反向散射系统进行的。为了解释非相干散射结果,建立了一个光谱参数库,该库给出了电离层参数范围广的非相干散射光谱的光谱宽度,光谱最大值和带限功率。有两种碰撞公式已被广泛用于减少D和E区域的非相干散射数据:Dougherty和Farley(1963)和Waldteufel(1970)。为了确定应使用哪种碰撞配方,我们检查了最近在未加热的电离层中进行的Arecibo实验的结果。从两种不同的碰撞配方得出的测得的电子-中性碰撞频率值与预测的模型值的比较表明,Dougherty和Farley配方的一致性极好,而Waldteufel配方的一致性差。使用Dougherty和Farley公式,我们从测得的加热到环境光谱参数之比确定电子温度变化。通过比较测得的电子温度变化与430 MHz加热的预测变化,我们发现D和E区域存在很大差异:测得的电子温度变化远小于预测值。可以通过将模型O(,2)旋转冷却速率增加10倍来消除75-100 km区域中的差异,而将75 km以下的差异可以增加4倍来消除。然而,冷却速度的提高并不是差异的唯一可能解释。如果在模型中显着增加了非麦克斯韦电子速度分布和热传导的其他两个影响,则可以消除差异。也可以通过使用f('2.18)频率缩放定律预测加热,而不是使用当前接受的f('2)定律来消除差异,但是没有物理解释支持这种修改。如果考虑D区域吸收,则3和5 MHz的加热结果与模型令人满意,因此不支持430 MHz结果所建议的增加的冷却速率。但是,其他建议的修改不会显着影响这些结果的一致性。还测量了由于52微秒诊断脉冲引起的发热。发现在70 km处进行诊断脉冲加热会使电子温度比环境温度高2.85(+ OR-)1.35。尽管误差估计很大,但是这种增加与模型的预测一致。

著录项

  • 作者

    COCO, DAVID STEPHEN.;

  • 作者单位

    Rice University.;

  • 授予单位 Rice University.;
  • 学科 Physics Atmospheric Science.
  • 学位 Ph.D.
  • 年度 1981
  • 页码 199 p.
  • 总页数 199
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 大气科学(气象学);
  • 关键词

  • 入库时间 2022-08-17 11:51:32

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号