来自GOCE卫星观测的热层纬向风的时空相关性

IF 2.6 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Ivana Molina, Ludger Scherliess
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引用次数: 1

摘要

热层风在高层大气动量和能量的传递中起着重要作用,并影响电离层等离子体的组成、动力学和形态。虽然风的一般形态已经被很好地理解了,但我们才刚刚开始理解它的可变性。在过去十年中,已经非常清楚的是,除了太阳对热层的强迫外,低层大气也是热层变率的一个重要驱动因素。因此,了解热层变率及其时空相关性对于提高对电离层-热层耦合系统及其与低层大气耦合的理解至关重要。从2009年11月到2013年10月,重力场和稳态海洋探测器(GOCE)提供了海拔约260公里的黎明和黄昏时分的纬向风。我们利用在地磁平静时期从低纬度到中纬度获得的GOCE纬向风观测资料,研究了黎明和黄昏前后纬向风的时空相关性。分别计算了2009 ~ 2012年12月至日各年GOCE纬向风的纬向相关性,建立了其年际变化规律。半球共轭点之间的相关性在中纬度地区发现。对2009年12月至日和2010年6月至日的纬度相关进行了比较,发现相关长度在冬半球的黎明和夏半球的黄昏期间始终较大。在2009年12月和2011年以及2010年6月也确定了纬向风的纵向/时间相关性,并发现经度/时间具有周期性。时间/纵向相关的时间演变在数天内逐渐减弱。相关系数的最大值总是出现在冬半球的黎明和夏半球的黄昏。在黎明期间,发现对时间/纵向相关性贡献最大的是非迁移潮汐,而在黄昏期间,额外的波浪似乎起着重要作用。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Spatial and temporal correlations of thermospheric zonal winds from GOCE satellite observations
Winds in the thermosphere play an important role in the transport of momentum and energy in the upper atmosphere and affect the composition, dynamics and morphology of the ionospheric plasma. Although the general morphology of the winds is well understood, we are only starting to understand its variability. During the last decade it has become inherently clear that in addition to solar forcing of the thermosphere, the lower atmosphere also is an important driver of thermospheric variability. Therefore, an understanding of thermospheric variability and its spatial and temporal correlations is critical for an improved understanding of the coupled ionosphere-thermosphere system and the coupling to the lower atmosphere. The Gravity Field and Steady-State Ocean Explorer (GOCE) provided zonal winds near dawn and dusk at an altitude of around 260 km from November 2009 to October 2013. We have used GOCE zonal wind observations from low- to mid-latitudes obtained during geomagnetically quiet times to investigate spatial and temporal correlations in the zonal winds near dawn and dusk. Latitudinal correlations were calculated for the GOCE zonal winds for December solstice separately for each year from 2009 to 2012 and their year-to-year variation was established. Correlations between hemispheric conjugate points were found at mid latitudes during the latter years. Latitudinal correlations for December solstice 2009 and June solstice 2010 were compared and the correlation length was found to be consistently larger in the winter hemisphere during dawn and in the summer hemisphere during dusk. Zonal wind longitudinal/temporal correlations were also determined for December 2009 and 2011 and for June 2010 and found to be periodic in longitude/time. The temporal evolution of the temporal/longitudinal correlations were found to gradually decrease over the course of several days. The maxima in the correlation coefficients were always located in the winter hemisphere during dawn and in the summer hemisphere during dusk. During dawn, the largest contributors to the temporal/longitudinal correlations were found to be nonmigrating tides, whereas during dusk, additional waves appear to play important roles.
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来源期刊
Frontiers in Astronomy and Space Sciences
Frontiers in Astronomy and Space Sciences ASTRONOMY & ASTROPHYSICS-
CiteScore
3.40
自引率
13.30%
发文量
363
审稿时长
14 weeks
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