Japan Geoscience Union Meeting 2025

Presentation information

[E] Oral

P (Space and Planetary Sciences ) » P-EM Solar-Terrestrial Sciences, Space Electromagnetism & Space Environment

[P-EM14] Study of coupling processes in solar-terrestrial system

Wed. May 28, 2025 10:45 AM - 12:15 PM 303 (International Conference Hall, Makuhari Messe)

convener:Mamoru Yamamoto(Research Institute for Sustainable Humanosphere, Kyoto University), Yasunobu Ogawa(National Institute of Polar Research), Satonori Nozawa(Institute for Space-Earth Environmental Research, Nagoya University), Akimasa Yoshikawa(Department of Earth and Planetary Sciences, Kyushu University), Chairperson:Yasunobu Ogawa(National Institute of Polar Research), Akimasa Yoshikawa(Department of Earth and Planetary Sciences, Kyushu University)

11:00 AM - 11:15 AM

[PEM14-08] Global Electric Field Response to the Development of High-Latitude Currents During Substorms

Moe Hayashi2, *Akimasa Yoshikawa1,4, Kaiki Yamaura3, Teji Uozumi4 (1.Department of Earth and Planetary Sciences, Fuculty of Science, Kyushu University, 2.Department of Earth and Planetary Sciences, Graduate School of Science, Kyushu University, 3.Department of Earth and Planetary Sciences, School of Science, Kyushu University, 4.International Center for Space and Planetary Science, Kyushu University)

Keywords:FAC development during auroral substorm, Ionospheric electric field responses during auroral substorm, Ampere satelite observation, Ground electric and magnetic fields observation

This study investigates the spatiotemporal evolution of high-latitude current systems during substorms using AMPERE and compares their characteristics with electric field responses in the mid- and equatorial latitudes on both the dayside and nightside.
There are two primary current systems in the polar ionosphere: Region 1 (R1) currents, linked to the magnetospheric convection, and Region 2 (R2) currents, linked to pressure gradient in the inner magnetosphere. When a substorm occurs due to plasma injection, plasma vortices at the edge of the plasma flow generate the substorm current wedge (SCW), which has the same current polarity as the R1 system. Previous studies have suggested that during the development and decline of these currents, R1 currents enhance the dawn-to-dusk penetration electric field, while R2 currents contribute to the dusk-to-dawn shielding effects, at the mid-, low- and equatorial latitudes. Additionally, the SCW also affects ionospheric currents on the dayside. However, the temporal and spatial evolution of these current systems during substorms and their effects on electric field responses at mid-latitudes and equatorial latitudes remain a controversial issue.
This study aims to elucidate the mechanisms driving electric field responses during substorms by examining the evolution of R1 and R2 currents, as well as the SCW, using AMPERE data. To achieve this, we investigate the temporal and spatial evolution of these currents and compare them with electric field responses in the mid- and equatorial ionosphere. As a case study, we focus on an isolated substorm that occurred at 15:03 UT on April 24, 2011.
Our analysis reveals that electric field responses on the dayside and nightside occur at different times, and the timing of each response corresponds to the development of high-latitude currents observed by AMPERE in their respective sectors. These results suggest that the observed electric fields in the dayside and nightside during substorms are driven by different current sources.