主要 SSW 事件期间温度变化和垂直传输的痕量物种对 MLT 区域结构的影响

IF 1.8 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS
Akash Kumar , M.V. Sunil Krishna , Alok Kumar Ranjan , Stefan Bender , Miriam Sinnhuber , Sumanta Sarkhel
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引用次数: 0

摘要

平流层突然变暖(SSW)事件是一种大尺度动态现象,会对不同大气层的环流、温度和成分产生重大影响。这些事件期间的环流变化会引起大气中性密度和离子密度的变化,并导致各种痕量物质的垂直传输。与低层大气相比,主要 SSW 事件在中间层和低温层(MLT)区域引起的影响的严重程度受到的关注较少。在两次平流层顶升高的重大 SSW 事件中,研究了温度和垂直传输的痕量物种对 MLT 区域的能量、热和成分结构的主要影响。一氧化氮体积发射率(NO-VER)是一氧化氮红外辐射冷却的测量指标,在 SSW 事件期间的动力学变化背景下首次报告了一氧化氮体积发射率的变化。这项研究调查了温度和一氧化氮的变化对多级层流区能量学的作用,特别是在形成抬升的平流层顶期间。在这些事件中,还研究了补充氮氧化物密度对二次臭氧层的影响,二次臭氧与氮氧化物之间的反相关性并不能断定氮氧化物在二次臭氧峰值密度变化中的作用。尽管 SSW 事件的定义特征相似,但它们对二次臭氧层的影响却不同。与之前的研究不同,有研究表明,在 SSW 事件期间,原子氧的可用性是导致观测到的二次臭氧变化的主要因素。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Influence of temperature changes and vertically transported trace species on the structure of MLT region during major SSW events

Sudden stratospheric warming (SSW) events are large-scale dynamic phenomena which can significantly affect the circulation, temperature, and composition of different atmospheric layers. The circulation changes during these events induce variations in the atmospheric neutral and ion densities and cause the vertical transport of various trace species. The severity of effects induced by major SSW events in the mesosphere and lower thermosphere (MLT) region has received less attention than that in the lower atmosphere. The major influence of temperature and vertically transported trace species on the energetics, thermal and compositional structure of the MLT region has been investigated during two major SSW events with elevated stratopause. Variations in the nitric oxide volume emission rates (NO-VER), a measure of infrared radiative cooling by NO, are reported for the first time in the context of the dynamical changes during SSW events. This study investigates the role of temperature and NO variability on the energetics of the MLT region, particularly during the formation of elevated stratopause. The effects of supplemented NO density on the secondary ozone layer has also been investigated during these events, the anti-correlation between secondary ozone and NO does not conclude on the role of NO in the secondary ozone peak density variations. Notwithstanding the similarity in terms of defining characteristics, both SSW events impact the secondary ozone layer differently. In contrast to earlier studies, it is suggested that along with temperature, the availability of atomic oxygen is the major factor for the observed variation in secondary ozone during the SSW events.

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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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