Evaluation of dB/dt amplitudes and sources over the Brazilian region during geomagnetic storms in the 2021–2022 biennium

IF 1.8 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS Journal of Atmospheric and Solar-Terrestrial Physics Pub Date : 2024-05-01 DOI:10.1016/j.jastp.2024.106196
G.B.D. Silva , L.R. Alves , K.V. Espinosa , V.M. Souza , L.A. da Silva , J.E.R. Costa , M.B. Pádua , S.A. Sanchez
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Abstract

The rate of change of the geomagnetic field (dB/dt) observed at Earth’s surface has been used as a proxy of geomagnetically induced currents, which are known to be hazardous for grounded technological systems such as high-voltage power grid systems. The dB/dt rates have been well characterized in the high latitude region (60°), but much less information is available for the low latitudes to date. To overcome this limitation, we have examined dB/dt rates on the H component of the geomagnetic field as measured by an array of stations operated by the EMBRACE Magnetometer Network in Brazil. The main focus is to characterize dB/dt occurrence at very low latitudes (22°) of the Brazilian peculiar territory, whose magnetic measurements are influenced by the equatorial electrojet and the presence of the South Atlantic Magnetic Anomaly (SAMA). The period investigated is from 2021 to 2022, over the ascending phase of the solar cycle 25. The statistical analysis demonstrates that dB/dt peak magnitudes are generally below 0.5 nT/s during magnetic storms, and exhibit a dependence on the solar cycle for the station near the center of the SAMA. However, we obtain for a particular case in 2021 that dB/dt reached 1.35 nT/s in magnitude at the magnetic equator during daytime, which is a significant value even for higher latitudes. A case study of the induced geoelectric fields during this event shows that the conductivity structure beneath two compared sites plays a major role in the amplitude of such fields than dB/dt amplitude. Also, the MLT distributions of dB/dt indicate that ultra-low frequency waves can be a major source of these signals in lower latitudes.

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评估 2021-2022 双年度地磁暴期间巴西地区的 dB/dt 幅值和来源
在地球表面观测到的地磁场变化率()已被用作地磁感应电流的代用指标,众所周知,地磁感应电流对高压电网系统等接地技术系统具有危险性。高纬度地区的地磁感应电流率已经有了很好的表征(),但迄今为止低纬度地区的地磁感应电流率信息要少得多。为了克服这一局限性,我们研究了巴西 EMBRACE 磁强计网络运行的台站阵列所测量的地磁场分量的速率。主要重点是描述巴西特殊地区极低纬度()的发生特征,其磁场测量受到赤道电射流和南大西洋磁异常(SAMA)的影响。研究时段为 2021 年至 2022 年,太阳周期 25 的上升阶段。统计分析表明,在磁暴期间,峰值幅度一般低于 0.5 nT/s,而在南大西洋磁异常中心附近的站点,峰值幅度则与太阳周期有关。不过,我们在 2021 年的一个特定案例中得到,白天在磁赤道的峰值达到 1.35 nT/s,即使在较高纬度地区也是一个重要值。对这一事件中的诱导地电场进行的案例研究表明,与振幅相比,两个对比地点下方的传导结构对这种地电场的振幅起着主要作用。此外,MLT 分布表明,超低频波可能是低纬度地区这些信号的主要来源。
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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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