Vishnu Rajendra Kumar, Richard L. Collins, Jintai Li, Rahsha Kerven, Jennifer Alspach, Denise Thorsen
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引用次数: 0
摘要
本研究介绍了阿拉斯加州查塔尼卡(65°N, 147°W)的Poker Flat Research Range (PFRR)的夜光云(nlc)和相关中间层条件的观测结果。从2005年到2022年,使用瑞利激光雷达系统测量了NLCs,在7月底到8月初共记录了28次事件。利用激光雷达数据的峰值散射系数和综合后向散射系数对云的亮度和持续时间进行了表征。利用流星雷达观测分析了当地的风型,而Aura MLS数据提供了NLC事件期间的温度和水蒸气剖面。结果表明,在Chatanika的NLC发生与相对于霜点的温度密切相关,并且表明最亮的NLC发生在MLS搭配表明在标准水平下的边缘亚饱和背景条件的时期。在Chatanika以北几百公里处存在有利的云层条件,流星雷达风支持了这一解释,表明向南的运输在将nlc运送到该地点方面发挥了主要作用。
An extended investigation of noctilucent cloud dynamics at Chatanika, Alaska using lidar, satellite, and radar observations
This study presents observations of noctilucent clouds (NLCs) and associated mesospheric conditions at Poker Flat Research Range (PFRR), Chatanika, Alaska (65° N, 147° W). NLCs were measured using the Rayleigh lidar system from 2005 to 2022, with a total of 28 events recorded between late July and early August. The clouds were characterized in terms of brightness and duration using the peak and integrated backscatter coefficients from lidar data. Local wind patterns were analyzed using meteor radar observations, while Aura MLS data provided temperature and water vapor profiles during the NLC events. The results show that NLC occurrence at Chatanika is strongly linked to temperatures relative to the frost point and indicate that the brightest NLCs occurred during periods when MLS collocations indicated marginally subsaturated background conditions at standard levels. Cloud-favorable conditions exist several hundred kilometers north of Chatanika, and meteor radar winds support this interpretation, suggesting that southward transport played a major role in delivering NLCs to the site.
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.