中间层和低层热层绝热变冷和变暖的估计

IF 1.8 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS
Jia Yue , Ningchao Wang
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引用次数: 0

摘要

利用利用宽带发射辐射测量(SABER)的大气探测技术,从全球平均CO2体积混合比(VMR)中测量CO2体积混合比(VMR)垂直位移,估算了中间层和低层热层(MLT)的绝热冷却和变暖。这项工作证实了夏季中流层温度在很大程度上是由绝热冷却控制的,而不是任何吸收加热或化学加热。本文还揭示了以前被忽视的在夏季绝热增温和冬季绝热降温的低层热层,由与冬夏环流相关的下行和上升流驱动。由于这一绝热变暖/冷却过程嵌入平均温度急剧上升的热层中,如果不去掉全球平均温度,它就不那么明显了。中间层温度则相反,缺乏强热源。夏季低层热层的加热异常(~ 100 K)很大。由于极光加热也发生在地磁极下热层,因此在未来的研究中应考虑下热层绝热变暖/冷却与极光加热之间的相互作用。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Estimation of adiabatic cooling and warming in the mesosphere and lower thermosphere
The adiabatic cooling and warming in the mesosphere and lower thermosphere (MLT) are estimated utilizing the Sounding of the Atmosphere using Broadband Emission Radiometry (SABER) measured CO2 volume mixing ratio (VMR) vertical displacement from the global mean CO2 VMR. This work confirms that the summer mesopause temperature is largely controlled by adiabatic cooling instead of any absorptive heating or chemical heating. The paper also reveals a previously overlooked layer of adiabatic warming in summer and adiabatic cooling in winter in the lower thermosphere, being driven by downwelling and upwelling associated with the winter-to-summer circulation. Since this adiabatic warming/cooling process is embedded in the thermosphere where the mean temperature rises sharply, it is not as distinct without removing the global mean temperature. The mesospheric temperature is the opposite, being lacking of strong heating sources. The heating anomaly (∼100 K) in the summer lower thermosphere is substantial. Because auroral heating also occurs in the geomagnetic polar lower thermosphere, the interaction between the adiabatic warming/cooling in the lower thermosphere and auroral heating should be considered in future studies.
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来源期刊
Journal of Atmospheric and Solar-Terrestrial Physics
Journal of Atmospheric and Solar-Terrestrial Physics 地学-地球化学与地球物理
CiteScore
4.10
自引率
5.30%
发文量
95
审稿时长
6 months
期刊介绍: The Journal of Atmospheric and Solar-Terrestrial Physics (JASTP) is an international journal concerned with the inter-disciplinary science of the Earth''s atmospheric and space environment, especially the highly varied and highly variable physical phenomena that occur in this natural laboratory and the processes that couple them. The journal covers the physical processes operating in the troposphere, stratosphere, mesosphere, thermosphere, ionosphere, magnetosphere, the Sun, interplanetary medium, and heliosphere. Phenomena occurring in other "spheres", solar influences on climate, and supporting laboratory measurements are also considered. The journal deals especially with the coupling between the different regions. Solar flares, coronal mass ejections, and other energetic events on the Sun create interesting and important perturbations in the near-Earth space environment. The physics of such "space weather" is central to the Journal of Atmospheric and Solar-Terrestrial Physics and the journal welcomes papers that lead in the direction of a predictive understanding of the coupled system. Regarding the upper atmosphere, the subjects of aeronomy, geomagnetism and geoelectricity, auroral phenomena, radio wave propagation, and plasma instabilities, are examples within the broad field of solar-terrestrial physics which emphasise the energy exchange between the solar wind, the magnetospheric and ionospheric plasmas, and the neutral gas. In the lower atmosphere, topics covered range from mesoscale to global scale dynamics, to atmospheric electricity, lightning and its effects, and to anthropogenic changes.
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