电离层对全球不同大洋盆地热带气旋的响应

IF 1.8 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS
Arup Patari , Anirban Guha
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引用次数: 0

摘要

研究了八个热带气旋(即伊欧塔、海马、哈罗德、威拉、安潘、伽伽、瓦德拉和布尔)对电离层的扰动,这八个热带气旋起源并生长于不同的海洋盆地。本研究使用了在阿加尔塔拉(AGT)运行的全球定位系统(GPS)总电子含量(TEC)接收器或气旋登陆区附近的不同国际全球导航卫星系统服务(IGS)站点提供的数据。尽管存在一些差异,但电离层对所有热带气旋的反应几乎相似。虽然在气旋风暴活跃阶段,地磁条件平静,没有任何其他地球物理现象造成的扰动,但在所有情况下,无论是登陆日还是次日,甚至是前一天,平均垂直电子总含量(VTEC)偏差都低于月平均值。北印度洋和南太平洋海盆上空的热带气旋的垂直总电子含量下降幅度较大。北大西洋和西北太平洋海盆上的气旋的垂直总电子含量值恢复较慢。北大西洋和西北太平洋海盆上空的热带气旋的垂直电子总含量值恢复较慢。但其他海盆上的热带气旋则恢复得很快。热带气旋(TC)的路径越长,垂直电子总含量(VTEC)值的下降幅度就越大。不同热带气旋的最大持续表面风速和总周期之间存在负相关,最低平均差值 VTEC 与前一天的差值也存在负相关。观测到的电离层反应异常可能是由于热带气旋引发的重力波、热带气旋终结者喷射出的中性粒子和闪电电场的共同作用造成的。为了解释热带气旋期间的对流活动,还考虑了外向长波辐射图。这项研究提供了有关区域特征的主要结果,从而为电离层对全球不同地理位置的不同热带气旋(TC)的响应提供了一个比较思路,这需要在未来进行进一步的全面调查。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Ionospheric responses to the tropical cyclones from different oceanic basins over the globe

The perturbations in the ionosphere due to eight tropical cyclones (TCs), namely Iota, Haima, Harold, Willa, Amphan, Gaja, Vadrah and Bulbul, originated and grown in different oceanic basins, are investigated. Total Electron Content (TEC) data, from Global Positioning System (GPS) TEC receiver in operation at Agartala (AGT) or different International GNSS Service (IGS) stations near the cyclone landfall regions, are used in this study. Despite some differences, the ionosphere responds to all tropical cyclones in an almost similar manner. Though the geomagnetic conditions are quiet and there are no perturbations due to any other geophysical phenomena in the active cyclonic storm stage, in all the cases there is a fall in average vertical total electron content (VTEC) deviations below the monthly mean value either on the landfall day or on the following day or even on just previous day. Decrements in Vertical Total Electron Content are found higher for tropical cyclones over North Indian and South Pacific oceanic basins. Recoveries in vertical total electron content values are slower for cyclones over the North Atlantic and North West Pacific basins. Recoveries in vertical total electron content (VTEC) values are slow for tropical cyclones (TCs) over the North Atlantic and North West Pacific basins. But those over other basins are quick. The longer the track of a tropical cyclone (TC), the higher is the reduction in the vertical total electron content (VTEC) value. A negative correlation exists between the maximum sustained surface wind velocities and the total periods of different TCs and also the difference of lowest average differential VTECs with that on the previous day. The observed anomaly in ionospheric responses might be due to the combined effect of TC-inspired gravity waves, ejection of neutral particles from the terminator of a tropical cyclone (TC) and lightning electric fields. To explain the observed results convective activities during TC, with the help of outgoing long wave radiation (OLR) map, are also taken into account. This study provides the primary results regarding regional characteristics and hence a comparative idea for the responses of the ionosphere to different tropical cyclones (TCs) from different geographical positions on the globe, which needs further comprehensive investigation in future.

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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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