TY - JOUR
T1 - Multi-Event Analysis of Magnetosphere-Ionosphere Coupling of Nighttime Medium-Scale Traveling Ionospheric Disturbances From the Ground and the Arase Satellite
AU - Kawai, K.
AU - Shiokawa, K.
AU - Otsuka, Y.
AU - Oyama, S.
AU - Connors, M. G.
AU - Kasahara, Y.
AU - Kasaba, Y.
AU - Nakamura, S.
AU - Tsuchiya, F.
AU - Kumamoto, A.
AU - Shinbori, A.
AU - Matsuoka, A.
AU - Shinohara, I.
AU - Miyoshi, Y.
N1 - Funding Information:
We thank Yasuo Katoh, Yoshiyuki Hamaguchi, Yuka Yamamoto, and Takumi Adachi, technical staff of the ISEE at Nagoya University, for their helpful support when installing the ground‐based airglow imagers at Athabasca, Gakona, and Kapuskasing. The airglow imagers installed are optically calibrated at the National Institute of Polar Research (Ogawa et al., 2020 ). Database construction for the PWING ground‐based instruments was supported by the ERG Science Center ( https://ergsc.isee.nagoya-u.ac.jp/ ) and the Inter‐university Upper atmosphere Global Observation Network (IUGONET) project ( http://www.iugonet.org/ ). Data from the PWING ground‐based instruments are available on these websites. Science data of the ERG (Arase) satellite were obtained from the ERG Science Center operated by ISAS/JAXA and ISEE/Nagoya University ( http://ergsc.isee.nagoya-u.ac.jp/ , see Miyoshi, Hori, et al., 2018 ). The Arase satellite datasets for this research are available in these in‐text data citation references: Kasahara, Kumamoto, et al. ( 2018 ), Kasahara, Kasaba, Matsuda, ( 2018 ), Matsuoka et al. ( 2018a , 2018b ). The Kp index data resources are available at https://www.gfz-potsdam.de/en/kp-index/ . This work was supported by 15H05815 (Y. Miyoshi), 16H06286 (K. Shiokawa and Y. Miyoshi), 20H01959 (Y. Miyoshi), 15H05747 (S. Oyama and Y. Miyoshi), 21H04518 (K. Shiokawa), JPJSBP120214805 (K. Shiokawa), and JPJSCCB20210003 (K. Shiokawa) of Japan Society for the Promotion of Science. The observatory housing the Athabasca instrument was constructed and is operated with funding from the Canada Foundation for Innovation and we thank Ian Schofield for assistance.
Funding Information:
We thank Yasuo Katoh, Yoshiyuki Hamaguchi, Yuka Yamamoto, and Takumi Adachi, technical staff of the ISEE at Nagoya University, for their helpful support when installing the ground-based airglow imagers at Athabasca, Gakona, and Kapuskasing. The airglow imagers installed are optically calibrated at the National Institute of Polar Research (Ogawa et al., 2020). Database construction for the PWING ground-based instruments was supported by the ERG Science Center (https://ergsc.isee.nagoya-u.ac.jp/) and the Inter-university Upper atmosphere Global Observation Network (IUGONET) project (http://www.iugonet.org/). Data from the PWING ground-based instruments are available on these websites. Science data of the ERG (Arase) satellite were obtained from the ERG Science Center operated by ISAS/JAXA and ISEE/Nagoya University (http://ergsc.isee.nagoya-u.ac.jp/, see Miyoshi, Hori, et al., 2018). The Arase satellite datasets for this research are available in these in-text data citation references: Kasahara, Kumamoto, et al. (2018), Kasahara, Kasaba, Matsuda, (2018), Matsuoka et al. (2018a, 2018b). The Kp index data resources are available at https://www.gfz-potsdam.de/en/kp-index/. This work was supported by 15H05815 (Y. Miyoshi), 16H06286 (K. Shiokawa and Y. Miyoshi), 20H01959 (Y. Miyoshi), 15H05747 (S. Oyama and Y. Miyoshi), 21H04518 (K. Shiokawa), JPJSBP120214805 (K. Shiokawa), and JPJSCCB20210003 (K. Shiokawa) of Japan Society for the Promotion of Science. The observatory housing the Athabasca instrument was constructed and is operated with funding from the Canada Foundation for Innovation and we thank Ian Schofield for assistance.
Publisher Copyright:
© 2023. American Geophysical Union. All Rights Reserved.
PY - 2023/2
Y1 - 2023/2
N2 - Kawai et al. (2021) reported the first ground-satellite conjugate observation of nighttime medium-scale traveling ionospheric disturbances (MSTIDs), by analyzing measurements from an airglow imager at Gakona (geographic latitude: 62.39°N, geographic longitude: 214.78°E, magnetic latitude: 63.60°N) and the Arase satellite in the magnetosphere on 3 November 2018. The Arase satellite observed variations in both the polarization electric field and the electron density as the Arase footprint passed through the MSTID structures in the ionosphere. In this study, we investigated whether these electric field and density variations associated with MSTIDs at subauroral latitudes are always observed by Arase in the magnetosphere. We used three airglow imagers installed at Gakona, Athabasca (geographic latitude: 54.60°N, geographic longitude: 246.36°E, magnetic latitude: 61.10°N), and Kapuskasing (geographic latitude: 49.39°N, geographic longitude: 277.81°E, magnetic latitude: 58.70°N) and the Arase satellite. We found eight observations of MSTIDs conjugate with Arase. They indicate that electric field and density variations associated with MSTIDs are not always observed in the magnetosphere. These variations tend to be observed in the magnetosphere during geomagnetically quiet times and when the amplitude of the MSTID is large. We categorized the MSTIDs into those caused by plasma instabilities and gravity waves and found that the electric field and density variations can be observed in the magnetosphere for both types of MSTIDs.
AB - Kawai et al. (2021) reported the first ground-satellite conjugate observation of nighttime medium-scale traveling ionospheric disturbances (MSTIDs), by analyzing measurements from an airglow imager at Gakona (geographic latitude: 62.39°N, geographic longitude: 214.78°E, magnetic latitude: 63.60°N) and the Arase satellite in the magnetosphere on 3 November 2018. The Arase satellite observed variations in both the polarization electric field and the electron density as the Arase footprint passed through the MSTID structures in the ionosphere. In this study, we investigated whether these electric field and density variations associated with MSTIDs at subauroral latitudes are always observed by Arase in the magnetosphere. We used three airglow imagers installed at Gakona, Athabasca (geographic latitude: 54.60°N, geographic longitude: 246.36°E, magnetic latitude: 61.10°N), and Kapuskasing (geographic latitude: 49.39°N, geographic longitude: 277.81°E, magnetic latitude: 58.70°N) and the Arase satellite. We found eight observations of MSTIDs conjugate with Arase. They indicate that electric field and density variations associated with MSTIDs are not always observed in the magnetosphere. These variations tend to be observed in the magnetosphere during geomagnetically quiet times and when the amplitude of the MSTID is large. We categorized the MSTIDs into those caused by plasma instabilities and gravity waves and found that the electric field and density variations can be observed in the magnetosphere for both types of MSTIDs.
KW - Arase
KW - MSTID
KW - field-line mapping
KW - ionosphere
KW - magnetosphere
KW - medium-scale traveling ionospheric disturbance
UR - http://www.scopus.com/inward/record.url?scp=85148890782&partnerID=8YFLogxK
U2 - 10.1029/2022JA030542
DO - 10.1029/2022JA030542
M3 - Journal Article
AN - SCOPUS:85148890782
SN - 2169-9380
VL - 128
JO - Journal of Geophysical Research: Space Physics
JF - Journal of Geophysical Research: Space Physics
IS - 2
M1 - e2022JA030542
ER -