TY - JOUR
T1 - Development of the Substorm as a Manifestation of Convection Transient
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, the authors used the high‐speed computing system at Polar Data Center of National Institute of Polar Research through General Collaboration Project 2–3, the KDK computer system at the Research Institute for Sustainable Humanosphere (RISH), Kyoto University through General Collaboration Project R2‐KDK‐03, and Nagoya University super computer system through Nagoya University High Performance Computing Research Project for Joint Computational Science in Japan. This study was supported by KAKENHI (JSPS KAKENHI Grant Number JP20H01960, Y. Ebihara) and KAKENHI (JSPS KAKENHI Grant Number JP20K03894, M. Watanabe).
Funding Information:
In the present study, the authors used the high-speed computing system at Polar Data Center of National Institute of Polar Research through General Collaboration Project 2?3, the KDK computer system at the Research Institute for Sustainable Humanosphere (RISH), Kyoto University through General Collaboration Project R2-KDK-03, and Nagoya University super computer system through Nagoya University High Performance Computing Research Project for Joint Computational Science in Japan. This study was supported by KAKENHI (JSPS KAKENHI Grant Number JP20H01960, Y. Ebihara) and KAKENHI (JSPS KAKENHI Grant Number JP20K03894, M. Watanabe).
Publisher Copyright:
© 2021. American Geophysical Union. All Rights Reserved.
PY - 2021/10
Y1 - 2021/10
N2 - We reproduced the substorm by global simulation and analyzed the development of convection, shear, the dynamo, and the field-aligned current (FAC) at the final stage of the growth phase. From these investigations, we show that the substorm is a manifestation of reconfiguration in global flow dynamics. Ionospheric convection can be understood from two aspects. One understanding is as the potential field generated by the FAC, and the other is as the projection of magnetospheric convection. In order for the two to coincide, the FAC must be transmitted together with the motion. As a consequence, the resulting convection must be continuous from the magnetosphere to the ionosphere. We see this connection from the drawing of shear to recognize that the substorm is the projection process of transient convection. In the growth phase, convective shear that causes the quiet arc and the Harang reversal (HR) occurs on the open/closed boundary along the surface of the plasma sheet with a continuous flow structure from the magnetosphere to the ionosphere. The onset starts from a more local flow that is induced by the near-earth neutral line (NENL). A narrow shear commences from the NENL in the mid-tail and extends to the ionosphere to replace growth phase shear. Along a closed magnetic field line connected to the NENL, direct penetration flow, squeezing flow, the near-earth dynamo, release of the HR, and the onset FAC occur successively and consequently cause the ground onset. Such onset mechanism is quite different from the model adopting the current wedge.
AB - We reproduced the substorm by global simulation and analyzed the development of convection, shear, the dynamo, and the field-aligned current (FAC) at the final stage of the growth phase. From these investigations, we show that the substorm is a manifestation of reconfiguration in global flow dynamics. Ionospheric convection can be understood from two aspects. One understanding is as the potential field generated by the FAC, and the other is as the projection of magnetospheric convection. In order for the two to coincide, the FAC must be transmitted together with the motion. As a consequence, the resulting convection must be continuous from the magnetosphere to the ionosphere. We see this connection from the drawing of shear to recognize that the substorm is the projection process of transient convection. In the growth phase, convective shear that causes the quiet arc and the Harang reversal (HR) occurs on the open/closed boundary along the surface of the plasma sheet with a continuous flow structure from the magnetosphere to the ionosphere. The onset starts from a more local flow that is induced by the near-earth neutral line (NENL). A narrow shear commences from the NENL in the mid-tail and extends to the ionosphere to replace growth phase shear. Along a closed magnetic field line connected to the NENL, direct penetration flow, squeezing flow, the near-earth dynamo, release of the HR, and the onset FAC occur successively and consequently cause the ground onset. Such onset mechanism is quite different from the model adopting the current wedge.
UR - http://www.scopus.com/inward/record.url?scp=85118186804&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=85118186804&partnerID=8YFLogxK
U2 - 10.1029/2020JA028942
DO - 10.1029/2020JA028942
M3 - Article
AN - SCOPUS:85118186804
SN - 2169-9380
VL - 126
JO - Journal of Geophysical Research: Space Physics
JF - Journal of Geophysical Research: Space Physics
IS - 10
M1 - e2020JA028942
ER -