Durga N. Kafle , Vincent B. Wickwar , Joshua P. Herron , Jonathan Price
{"title":"Characteristics of monochromatic gravity waves in the mesosphere observed by Rayleigh lidar above Logan, Utah","authors":"Durga N. Kafle , Vincent B. Wickwar , Joshua P. Herron , Jonathan Price","doi":"10.1016/j.jastp.2024.106329","DOIUrl":null,"url":null,"abstract":"<div><p>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 <span><math><mrow><msub><mi>λ</mi><mi>z</mi></msub></mrow></math></span> ranged over 6–19 km with 12–14 km the most prevalent and the measured wave period <span><math><mrow><mi>τ</mi></mrow></math></span> ranged over 2–8 h with 5–6 h the most prevalent. The values of <span><math><mrow><msub><mi>λ</mi><mi>z</mi></msub></mrow></math></span>, <span><math><mrow><mi>τ</mi></mrow></math></span> and mean wind velocity <em>u</em> were used to infer vertical phase velocities <span><math><mrow><msub><mi>c</mi><mi>z</mi></msub></mrow></math></span>, horizontal wavelengths <span><math><mrow><msub><mi>λ</mi><mi>x</mi></msub></mrow></math></span>, horizontal phase velocities <span><math><mrow><msub><mi>c</mi><mi>x</mi></msub></mrow></math></span> and horizontal distances to the source region <em>x</em>. There appears to be a clear seasonal dependence in <span><math><mrow><msub><mi>c</mi><mi>z</mi></msub></mrow></math></span>, <span><math><mrow><mi>τ</mi></mrow></math></span>, <span><math><mrow><msub><mi>c</mi><mi>x</mi></msub></mrow></math></span>, <span><math><mrow><msub><mi>λ</mi><mi>x</mi></msub></mrow></math></span>, and <em>x</em> but not in <span><math><mrow><msub><mi>λ</mi><mi>z</mi></msub></mrow></math></span>. The <span><math><mrow><msub><mi>c</mi><mi>z</mi></msub></mrow></math></span> values maximize in summer, <span><math><mrow><mi>τ</mi></mrow></math></span> and <em>x</em> maximize in winter whereas <span><math><mrow><msub><mi>c</mi><mi>x</mi></msub></mrow></math></span> and <span><math><mrow><msub><mi>λ</mi><mi>x</mi></msub></mrow></math></span>, maximize in winter and summer but minimize in spring and autumn. The values of <em>x</em> 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.</p></div>","PeriodicalId":15096,"journal":{"name":"Journal of Atmospheric and Solar-Terrestrial Physics","volume":"263 ","pages":"Article 106329"},"PeriodicalIF":1.8000,"publicationDate":"2024-08-10","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.sciencedirect.com/science/article/pii/S1364682624001573/pdfft?md5=cc36af67f5be852f1b47386f6286d986&pid=1-s2.0-S1364682624001573-main.pdf","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Atmospheric and Solar-Terrestrial Physics","FirstCategoryId":"89","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S1364682624001573","RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"GEOCHEMISTRY & GEOPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
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 ranged over 6–19 km with 12–14 km the most prevalent and the measured wave period ranged over 2–8 h with 5–6 h the most prevalent. The values of , and mean wind velocity u were used to infer vertical phase velocities , horizontal wavelengths , horizontal phase velocities and horizontal distances to the source region x. There appears to be a clear seasonal dependence in , , , , and x but not in . The values maximize in summer, and x maximize in winter whereas and , 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.
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.