{"title":"Evaluation of dB/dt amplitudes and sources over the Brazilian region during geomagnetic storms in the 2021–2022 biennium","authors":"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","doi":"10.1016/j.jastp.2024.106196","DOIUrl":null,"url":null,"abstract":"<div><p>The rate of change of the geomagnetic field (<span><math><mrow><mi>d</mi><mi>B</mi><mo>/</mo><mi>d</mi><mi>t</mi></mrow></math></span>) 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 <span><math><mrow><mi>d</mi><mi>B</mi><mo>/</mo><mi>d</mi><mi>t</mi></mrow></math></span> rates have been well characterized in the high latitude region (<span><math><mrow><mo>≳</mo><mn>60</mn><mo>°</mo></mrow></math></span>), but much less information is available for the low latitudes to date. To overcome this limitation, we have examined <span><math><mrow><mi>d</mi><mi>B</mi><mo>/</mo><mi>d</mi><mi>t</mi></mrow></math></span> rates on the <span><math><mi>H</mi></math></span> 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 <span><math><mrow><mi>d</mi><mi>B</mi><mo>/</mo><mi>d</mi><mi>t</mi></mrow></math></span> occurrence at very low latitudes (<span><math><mrow><mo>≲</mo><mn>22</mn><mo>°</mo></mrow></math></span>) 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 <span><math><mrow><mi>d</mi><mi>B</mi><mo>/</mo><mi>d</mi><mi>t</mi></mrow></math></span> 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 <span><math><mrow><mi>d</mi><mi>B</mi><mo>/</mo><mi>d</mi><mi>t</mi></mrow></math></span> 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 <span><math><mrow><mi>d</mi><mi>B</mi><mo>/</mo><mi>d</mi><mi>t</mi></mrow></math></span> amplitude. Also, the MLT distributions of <span><math><mrow><mi>d</mi><mi>B</mi><mo>/</mo><mi>d</mi><mi>t</mi></mrow></math></span> indicate that ultra-low frequency waves can be a major source of these signals in lower latitudes.</p></div>","PeriodicalId":15096,"journal":{"name":"Journal of Atmospheric and Solar-Terrestrial Physics","volume":null,"pages":null},"PeriodicalIF":1.8000,"publicationDate":"2024-05-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://www.sciencedirect.com/science/article/pii/S1364682624000245/pdfft?md5=927fa34b9520803ef821e3ccd2628cda&pid=1-s2.0-S1364682624000245-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/S1364682624000245","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
The rate of change of the geomagnetic field () 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 rates have been well characterized in the high latitude region (), but much less information is available for the low latitudes to date. To overcome this limitation, we have examined rates on the 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 occurrence at very low latitudes () 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 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 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 amplitude. Also, the MLT distributions of indicate that ultra-low frequency waves can be a major source of these signals in lower latitudes.
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.