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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Decadal Solar-Cycle Conseact,以及基于Simed测量的STRATHEBER,Messehery和Lower Thermosphere的昼夜变化的关系

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摘要

There is evidence that the ozone and temperature responses to the solar cycle of ~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 ~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 ~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 ~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,臭氧和温度响应到〜11的太阳循环依赖于当地的测量时间。在这里,我们以完全可用的全部昼夜循环,基于SABRER数据呈现相关结果。在该领域,几乎所有使用的卫星数据都仅在一个或两个固定的本地时间测量,这可能在各种卫星之间不同。因此,根据具体数据集,响应的估计可以不同。此外,多年来,由于轨道漂移,一些卫星测量的当地时间也漂移。相比之下,SABER在各种当地时间进行测量,提供了在24小时内估计昼夜变化的机会。然后,我们还可以在昼夜周期和固定的当地卫星数据的固定本地时间进行估计对太阳循环的响应进行比较。基于SABER测量的分解手段,在本研究中得出的反应与先前的研究基于来自哈吞曲仪的数据,这仅在日出和日落时测量数据,从而支持对这两项研究的分析。我们发现,对于高于〜40km的臭氧,区间意味着反映特定的本地时间(例如,6,12,18,24 LST - 本地太阳时间)导致对响应的不同值,以及基于区域的不同响应平均在24小时本地时间段,如在3-D模型中。对于温度,即使在〜30公里和以上,昼夜变化对响应的影响并不可忽略。我们还考虑了由于某些操作卫星的轨道漂移而导致局部时间变化的后果,并且对于臭氧和温度,它们的效果可以高于〜30公里。以前基于其他卫星数据的研究没有描述当地时间的治疗,如果有的话。有些研究还分析了从不同来源合并的数据,在不同的当地时间进行了测量。通常,这些研究的结果并不完全同意。虽然响应是昼夜变异的函数,但这并不是说他们是差异的主要原因,因为有可能其他数据有关的问题。由于卫星轨道漂移引起的影响可能在响应中解释一些意外变化,特别是高于40公里。

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