首页> 外文期刊>Annales Geophysicae >Ozone and temperature decadal solar-cycle responses, and their relation to diurnal variations in the stratosphere, mesosphere, and lower thermosphere, based on measurements from SABER on TIMED
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Ozone and temperature decadal solar-cycle responses, and their relation to diurnal variations in the stratosphere, mesosphere, and lower thermosphere, based on measurements from SABER on TIMED

机译:臭氧和温度的年代际太阳循环响应及其与平流层,中层和较低热层日变化的关系,基于TIME的SABER测量

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摘要

There is evidence that the ozone and temperature responses to the solar cycle of similar to 11 years depend on the local times of measurements. Here we present relevant results based on SABER data over a full diurnal cycle, which were not previously available. In this area, almost all satellite data used are measured at only one or two fixed local times, which can differ among various satellites. Consequently, estimates of responses can be different depending on the specific data set. Furthermore, over years, due to orbital drift, the local times of the measurements of some satellites have also drifted. In contrast, SABER makes measurements at various local times, providing the opportunity to estimate diurnal variations over 24 h. We can then also estimate responses to the solar cycle over both a diurnal cycle and at the fixed local times of specific satellite data for comparison. Responses derived in this study, based on zonal means of SABER measurements, agree favorably with previous studies based on data from the HALOE instrument, which only measured data at sunrise and sunset, thereby supporting the analysis of both studies. We find that for ozone above similar to 40 km, zonal means reflecting specific local times (e.g., 6, 12, 18, 24 LST - local solar time) lead to different values of responses, and to different responses based on zonal means that are also averages over the 24 h local time period, as in 3-D models. For temperature, the effects of diurnal variations on the responses are not negligible even at similar to 30 km and above. We also considered the consequences of local time variations due to orbital drifts of certain operational satellites, and, for both ozone and temperature, their effects can be significant above similar to 30 km. Previous studies based on other satellite data do not describe the treatment, if any, of local times. Some studies also analyzed data merged from different sources, with measurements made at different local times. Generally, the results of these studies do not agree very well among themselves. Although responses are a function of diurnal variations, this is not to say that they are the major reason for the differences, as there are likely other data-related issues. The effects due to satellite orbital drift may explain some unexpected variations in the responses, especially above 40 km.
机译:有证据表明,臭氧和温度对太阳周期的响应大约为11年,取决于当地的测量时间。在此,我们基于整个昼夜周期内的SABRE数据提供了相关结果,而以前没有这些结果。在该地区,几乎所有使用的卫星数据仅在一个或两个固定的本地时间进行测量,不同的卫星之间可能有所不同。因此,响应的估计可能会有所不同,具体取决于特定的数据集。此外,多年来,由于轨道漂移,一些卫星的测量本地时间也已漂移。相比之下,SABRE在各个本地时间进行测量,从而提供了估算24小时内昼夜变化的机会。然后,我们还可以估算昼夜周期和特定卫星数据的固定本地时间对太阳周期的响应,以进行比较。本研究基于SABER测量的区域平均值得出的响应与基于HALOE仪器数据的先前研究相吻合,后者仅在日出和日落时测量数据,从而支持两项研究的分析。我们发现,对于高于40 km的臭氧,反映特定当地时间(例如6、12、18、24 LST-当地太阳时间)的纬向平均值会导致不同的响应值,并且基于纬向平均值会导致不同的响应。像3-D模型一样,也可以在24小时本地时间段取平均值。对于温度,即使在大约30 km及以上,昼夜变化对响应的影响也不能忽略。我们还考虑了某些操作卫星的轨道漂移引起的当地时间变化的后果,并且对于臭氧和温度而言,它们的影响在超过30 km时可能会很大。先前基于其他卫星数据的研究没有描述当地时间的处理方式(如果有)。一些研究还分析了来自不同来源的合并数据,并在不同的本地时间进行了测量。通常,这些研究的结果彼此之间并不十分吻合。尽管响应是日变化的函数,但这并不是说它们是差异的主要原因,因为可能还会存在其他与数据相关的问题。卫星轨道漂移引起的影响可能解释了响应中的某些意外变化,尤其是在40 km以上。

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  • 来源
    《Annales Geophysicae》 |2019年第4期|471-485|共15页
  • 作者

    Huang Frank T.; Mayr Hans G.;

  • 作者单位

    Univ Maryland Baltimore Cty Baltimore MD 21250 USA;

    NASA Goddard Space Flight Ctr Greenbelt MD 20771 USA;

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  • 正文语种 eng
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