Variation of the H Component of Geomagnetic Field: Relationship to the Ring and Field Aligned Currents

IF 0.5 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS Kinematics and Physics of Celestial Bodies Pub Date : 2023-03-20 DOI:10.3103/S0884591323010063
Sabin Gautam, Sarup Khadka Saurav, Binod Adhikari, Santosh Sapkota, Parashu Ram Poudel, Roshan Kumar Mishra, Chhabi Kumar Shrestha
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Abstract

Disturbance of equatorial ring current during the geomagnetic storm has dominant effect on geomagnetic field. The short term irregular variation on geomagnetic field is characterized by interaction of solar-wind magnetic field and Earth’s magnetosphere, which develops time varying current in magnetosphere and ionosphere. This study represents the irregular variation on H component of Earth’s magnetic field during three intense geomagnetic storm events. Among the five selected stations, four are at low-latitude and remaining one is at middle latitude. All the stations recorded the maximum depression on H component during the main phase of storm but sudden storm commencements (SSCs) event before initial phase caused slight increase in magnitude. In each of the event, low-latitude stations recorded large perturbation on magnetic field as compared to the middle latitude station. This result supports the intensification of ring current as initiated by the transfer of plasma and energy through interplanetary coronal mass ejections (ICMEs) and finally causes falling off of H component. Kakadu station (southern latitude) showed maximum value of ΔH in second and third event, this result keeps up that mostly southern hemisphere station measures large decline on H component during storm time. The calculated value of ring current and field aligned current (FAC) showed extreme negative correlation with ΔH. This unique result reveals that ring current is not only a factor that cause disturbance on horizontal component of Earth’s magnetic field but FAC also has considerable effect.

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地磁场H分量的变化:与环和场向电流的关系
地磁风暴期间赤道环流扰动对地磁场的影响占主导地位。地磁场的短期不规则变化以太阳风磁场与地球磁层相互作用为特征,在磁层和电离层中形成时变电流。本文研究了三次强地磁风暴期间地球磁场H分量的不规则变化。在选定的5个站点中,4个位于低纬度,1个位于中纬度。各台站在风暴主阶段H分量下降最大,但在风暴初始阶段之前的风暴突发事件使H分量略有增加。在每次事件中,低纬度台站记录到的磁场扰动都比中纬度台站大。这一结果支持了环电流的增强是由等离子体和能量通过行星际日冕物质抛射(ICMEs)转移引起的,并最终导致H分量的脱落。Kakadu台站(南纬)在第2次和第3次的H分量值最大,这一结果支持了大部分南半球台站在风暴期间测得的H分量下降较大。环形电流和场向电流(FAC)的计算值与ΔH呈极负相关。这一独特的结果表明,环电流不仅是对地磁场水平分量产生扰动的一个因素,而且FAC也有相当大的影响。
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来源期刊
Kinematics and Physics of Celestial Bodies
Kinematics and Physics of Celestial Bodies ASTRONOMY & ASTROPHYSICS-
CiteScore
0.90
自引率
40.00%
发文量
24
审稿时长
>12 weeks
期刊介绍: Kinematics and Physics of Celestial Bodies is an international peer reviewed journal that publishes original regular and review papers on positional and theoretical astronomy, Earth’s rotation and geodynamics, dynamics and physics of bodies of the Solar System, solar physics, physics of stars and interstellar medium, structure and dynamics of the Galaxy, extragalactic astronomy, atmospheric optics and astronomical climate, instruments and devices, and mathematical processing of astronomical information. The journal welcomes manuscripts from all countries in the English or Russian language.
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