TY - JOUR
T1 - Formation of a 3-D Oscillatory Current System Associated With Global High-Correlation Pi 2 Event
T2 - A Case Study
AU - Uozumi, T.
AU - Yoshikawa, A.
AU - Ohtani, S.
N1 - Funding Information:
GOES 12 magnetic field data are open data for scientific use; those were provided at the website of https://cdaweb.sci.gsfc.nasa.gov/index.html/. THEMIS data were provided at the website of https://cdaweb.sci.gsfc.nasa.gov/index.html/. MAGDAS/CPMN magnetic data were provided by the principle investigator of the MAGDAS/CPMN Project (http://data.icswse.kyushu-u.ac.jp/). This MAGDAS/CPMN observation was made by the financial supports of Japan Society for the Promotion of Science (JSPS) as Grant-in-Aid for Overseas Scientific Survey (15253005 and 18253005) and for Publication of Scientific Research Results (188068, 198055, and 208043). The MAGDAS/CPMN database was made by the financial supports of National Institute of Information and Communications Technology (NiCT) as the funded research. The MAGDAS/CPMN data have been processed and calibrated at International Center for Space Weather Science and Education, Kyushu University. This work was supported in part by JSPS Core-to-Core Program (B. Asia-Africa Science Platforms), Formation of Preliminary Center for Capacity Building for Space Weather Research. This work was supported by MEXT/JSPS KAKENHI Grant 15H05815. Work at JHU/APL was supported by NASA Grant NNX16AF74G and National Science Foundation (NSF) Grant 1603028. This work was carried out by the joint research program of the Institute for Space-Earth Environmental Research (ISEE), Nagoya University. This study was also supported by National Institute of Polar Research (NIPR) through General Collaboration Project*1no. 29-19.
Publisher Copyright:
©2019. American Geophysical Union. All Rights Reserved.
PY - 2020/1/1
Y1 - 2020/1/1
N2 - We present a typical example of the formation of a three-dimensional (3-D) oscillatory current system associated with a global high-correlation Pi 2 event. The time variation of the field-aligned current (FAC) density in the magnetosphere is estimated using multisatellite magnetic field data in the near-Earth plasma sheet (~10 RE, ~23 MLT). Pi 2 pulsations, which were accompanied with the development of the upward and downward FACs in the substorm current wedge, were observed at mid-latitude stations in the pre-midnight sector (20.6 and 22.6 MLT), and the periodicity of the FAC fluctuations was correlated with the estimated current-density fluctuations in the near-Earth plasma sheet. Compressional signals of the Pi 2 pulsation were observed by an equatorial ground station and a geosynchronous satellite located in the midnight sector (0.1 and 0.4 MLT). A detailed comparison of the Pi 2 waveforms, which were simultaneously observed on the ground and in the near-Earth magnetosphere, revealed high correlations between the fluctuations of the FACs and compressional pulses. These observations strongly suggest the formation of a 3-D oscillatory current system associated with the global high-correlation Pi 2 event. The sources of the oscillatory current system and compressional pulses were confirmed to be closely coupled with one another.
AB - We present a typical example of the formation of a three-dimensional (3-D) oscillatory current system associated with a global high-correlation Pi 2 event. The time variation of the field-aligned current (FAC) density in the magnetosphere is estimated using multisatellite magnetic field data in the near-Earth plasma sheet (~10 RE, ~23 MLT). Pi 2 pulsations, which were accompanied with the development of the upward and downward FACs in the substorm current wedge, were observed at mid-latitude stations in the pre-midnight sector (20.6 and 22.6 MLT), and the periodicity of the FAC fluctuations was correlated with the estimated current-density fluctuations in the near-Earth plasma sheet. Compressional signals of the Pi 2 pulsation were observed by an equatorial ground station and a geosynchronous satellite located in the midnight sector (0.1 and 0.4 MLT). A detailed comparison of the Pi 2 waveforms, which were simultaneously observed on the ground and in the near-Earth magnetosphere, revealed high correlations between the fluctuations of the FACs and compressional pulses. These observations strongly suggest the formation of a 3-D oscillatory current system associated with the global high-correlation Pi 2 event. The sources of the oscillatory current system and compressional pulses were confirmed to be closely coupled with one another.
UR - http://www.scopus.com/inward/record.url?scp=85081403342&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=85081403342&partnerID=8YFLogxK
U2 - 10.1029/2019JA026988
DO - 10.1029/2019JA026988
M3 - Article
AN - SCOPUS:85081403342
SN - 2169-9380
VL - 125
JO - Journal of Geophysical Research: Space Physics
JF - Journal of Geophysical Research: Space Physics
IS - 1
M1 - e2019JA026988
ER -