TY - JOUR
T1 - Reproduction of Ground Magnetic Variations During the SC and the Substorm From the Global Simulation and Biot-Savart's Law
AU - Tanaka, T.
AU - Ebihara, Y.
AU - Watanabe, M.
AU - Den, M.
AU - Fujita, S.
AU - Kikuchi, T.
AU - Hashimoto, K. K.
AU - Kataoka, R.
N1 - Funding Information:
In the present study, we used the high-speed computing system at Polar Data Center of National Institute of Polar Research through General Collaboration Project 29-5, and the KDK computer system at the Research Institute for Sustainable Humanosphere (RISH), Kyoto University through General Collaboration Project 2019KDK-04. This study was supported by KAKENHI (Grant 15H03732) and MEXT/JSPS KAKENHI Grant 15H05815. Numerical data (coordinate data and variable data), information for graphic program, and history data necessary to reproduce drawings are available online (http://polaris.nipr.ac.jp/~reppu/reppu2/reppu6/).
Publisher Copyright:
©2020. American Geophysical Union. All Rights Reserved.
PY - 2020/2/1
Y1 - 2020/2/1
N2 - In this paper, currents causing the sudden commencement (SC), the AU/AL indices, and the positive bay during the substorm are identified from the global simulation and Biot-Savart's law. Candidate currents assumed as causes of these ground magnetic variations are the ionospheric Hall current, the ionospheric Pedersen current, the field-aligned current (FAC), and other magnetospheric currents than the FAC. In general, FAC effect and Pedersen current effect cancel out each other under the restriction of Fukushima's theorem. During the SC, for instance, the midlatitude preliminary positive impulse appears in the prenoon and midlatitude preliminary reverse impulse (PRI) appears in the postnoon, due to the remaining effect of the Hall current. However, violations of the Fukushima's theorem are also common such as in the cases of the equatorial PRI, the auroral electrojet, and the positive bay. The equatorial PRI caused by the Pedersen current appears both in the prenoon and postnoon regions. In the auroral region, the Hall current effect prevails over other currents so much and determines the AU/AL indices only from it regardless other currents. The midlatitude positive bay on the nightside is generated by the effect of the FAC. From these diverse reproduction of ground magnetic variations, a further verification is given for the global simulation in reproductions of the magnetosphere-ionosphere coupling process.
AB - In this paper, currents causing the sudden commencement (SC), the AU/AL indices, and the positive bay during the substorm are identified from the global simulation and Biot-Savart's law. Candidate currents assumed as causes of these ground magnetic variations are the ionospheric Hall current, the ionospheric Pedersen current, the field-aligned current (FAC), and other magnetospheric currents than the FAC. In general, FAC effect and Pedersen current effect cancel out each other under the restriction of Fukushima's theorem. During the SC, for instance, the midlatitude preliminary positive impulse appears in the prenoon and midlatitude preliminary reverse impulse (PRI) appears in the postnoon, due to the remaining effect of the Hall current. However, violations of the Fukushima's theorem are also common such as in the cases of the equatorial PRI, the auroral electrojet, and the positive bay. The equatorial PRI caused by the Pedersen current appears both in the prenoon and postnoon regions. In the auroral region, the Hall current effect prevails over other currents so much and determines the AU/AL indices only from it regardless other currents. The midlatitude positive bay on the nightside is generated by the effect of the FAC. From these diverse reproduction of ground magnetic variations, a further verification is given for the global simulation in reproductions of the magnetosphere-ionosphere coupling process.
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U2 - 10.1029/2019JA027172
DO - 10.1029/2019JA027172
M3 - Article
AN - SCOPUS:85086485471
SN - 2169-9380
VL - 125
JO - Journal of Geophysical Research: Space Physics
JF - Journal of Geophysical Research: Space Physics
IS - 2
M1 - e2019JA027172
ER -