与强烈地磁暴相关的低纬度地磁响应:墨西哥的区域空间天气

IF 1.8 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS Journal of Atmospheric and Solar-Terrestrial Physics Pub Date : 2024-04-20 DOI:10.1016/j.jastp.2024.106237
C.I. Castellanos-Velazco , P. Corona-Romero , J.A. González-Esparza , M.A. Sergeeva , A.L. Caccavari-Garza , V.J. Gatica-Acevedo
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引用次数: 0

摘要

在这项工作中,我们研究了墨西哥中部空间天气的区域表现形式,将当地地磁反应与其行星对应物分离开来。为此,我们分析了 20 次强烈地磁暴,确定了 Teoloyucan 磁性观测站(位于墨西哥城北部)记录的区域地磁数据中电离层的贡献。我们的分析表明,当地地磁响应主要由电离层扰动驱动。我们还发现,2 号扰动极地电流和扰动动力电流与区域地磁响应特别相关。此外,我们还发现,区域地磁活动可以近似地由行星地磁响应和电离层扰动电流引起的区域磁扰动的综合效应所决定。最后,我们的研究结果凸显了地磁响应在区域尺度上的特殊性。
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Low latitude geomagnetic response associated with intense geomagnetic storms: Regional space weather in Mexico

In this work we studied the regional manifestations of space weather at central Mexico through isolate the local geomagnetic response from its planetary counterpart. In order to do so, we analyzed 20 intense geomagnetic storms by identifying the ionospheric contribution in their regional geomagnetic data as registered at the Magnetic Observatory of Teoloyucan (located at the north of Mexico City). Our analysis indicated that local geomagnetic response is mainly driven by ionospheric disturbances. We also found that the disturbed polar current number 2 and the disturbed dynamo current are particularly relevant for the regional geomagnetic response. Additionally, we showed that regional geomagnetic activity can be approximated by the combined effects of the planetary geomagnetic response and the regional magnetic perturbations induced by the commented ionospheric currents. Finally, our results highlights the particularities that geomagnetic response has at regional scales.

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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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