犹他州洛根上空雷利激光雷达观测到的中间层单色重力波的特征

IF 1.8 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS
Durga N. Kafle , Vincent B. Wickwar , Joshua P. Herron , Jonathan Price
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引用次数: 0

摘要

利用在美国犹他州洛根(北纬 41.7 度,西经 111.8 度)上空收集的 11 年雷利激光雷达数据,对 45-90 千米高度范围内的大气重力波(AGW)特征进行了研究。用 3 千米垂直分辨率和 10 分钟时间分辨率获得的相对密度扰动变化来确定整个中间层是否存在单色重力波特征。测得的垂直波长 λz 在 6 至 19 千米之间,其中以 12 至 14 千米最为普遍;测得的波周期 τ 在 2-8 小时之间,其中以 5 至 6 小时最为普遍。利用 λz、τ 和平均风速 u 的值推断垂直相位速度 cz、水平波长 λx、水平相位速度 cx 和到源区的水平距离 x。cz 值在夏季最大,τ 和 x 在冬季最大,而 cx 和 λx 在冬季和夏季最大,但在春季和秋季最小。对于 60 千米处的波浪,x 的取值范围为 1300-5000 千米;对于 90 千米处的波浪,x 的取值范围为 2000-7500 千米。因此,这些 AGW 的源头很远。此外,要使这些单色波整夜存在或看起来延伸到 45-90 千米,它必须来自一个非常延伸的区域并持续很长时间。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Characteristics of monochromatic gravity waves in the mesosphere observed by Rayleigh lidar above Logan, Utah

Atmospheric gravity wave (AGW) characteristics were examined using Rayleigh lidar data collected over a period spanning 11 years above Logan, UT (41.7°N, 111.8°W), over an altitude range of 45–90 km. Variations of the relative density perturbations obtained with 3-km vertical resolution and 10-min temporal resolution are used to identify the presence of monochromatic gravity wave features throughout the mesosphere. The measured vertical wavelengths λz ranged over 6–19 km with 12–14 km the most prevalent and the measured wave period τ ranged over 2–8 h with 5–6 h the most prevalent. The values of λz, τ and mean wind velocity u were used to infer vertical phase velocities cz, horizontal wavelengths λx, horizontal phase velocities cx and horizontal distances to the source region x. There appears to be a clear seasonal dependence in cz, τ, cx, λx, and x but not in λz. The cz values maximize in summer, τ and x maximize in winter whereas cx and λx, maximize in winter and summer but minimize in spring and autumn. The values of x ranged over 1300–5000 km for waves at 60 km and ∼2000–7500 km for waves at 90 km. The source of these AGWs is, thus, far away. Furthermore, for one of these monochromatic waves to exist all night or appear to extend over 45–90 km, it has to originate from a very extended region and persist for a long time.

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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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