TY - JOUR
T1 - Observations of Low-Latitude Traveling Ionospheric Disturbances by a 630.0-nm Airglow Imager and the CHAMP Satellite Over Indonesia
AU - Moral, Aysegul Ceren
AU - Shiokawa, Kazuo
AU - Suzuki, Shin
AU - Liu, Huixin
AU - Otsuka, Yuichi
AU - Yatini, Clara Yoko
N1 - Funding Information:
We thank Y. Katoh, M. Satoh, Y. Yamamoto, and Y. Hamaguchi of the Institute for Space-Earth Environmental Research Laboratory (ISEE), Nagoya University, for their helpful support at the all-sky imager at Kototabang. The ISEE, the Research Institute for Sustainable Humanosphere, Kyoto University, Japan, and the National Institute of Aeronautical and Space Science, Indonesia, carried out airglow observations at Kototabang. We want to thank to Space Agency of the German Aerospace Center (DLR) and the project director H. Lühr for the CHAMP mission. This work was supported by Grants-in-Aid for Scientific Research (13573006, 20244080, 16H06286, and 15H05815), a Grant-in-Aid for Scientific Research in Priority Areas (764), and the JSPS Core-to-Core Program B, Asia-Africa Science Platforms. Huixin Liu is supported by JSPS KAKEN HI grants 18H01270, 18H04446, and 17KK0095. Aysegul Ceren Moral is supported by a research scholarship from the Ministry of Education, Culture, Sports, Science and Technology, Japan. Data set can be downloaded from Zenodo website (http://doi.org/10.5281/zenodo.1243819).
Publisher Copyright:
© 2019. American Geophysical Union. All Rights Reserved.
PY - 2019/3
Y1 - 2019/3
N2 - We report the first comparison of ground and satellite measurements of low-latitude traveling ionospheric disturbances (TIDs). Three TID events were simultaneously observed by a 630.0-nm airglow imager and the CHAllenging Minisatellite Payload (CHAMP) satellite at Kototabang, Indonesia (geographic coordinates: 0.2° S, 100.3° E, geomagnetic latitude: 10.6° S). In 630.0-nm airglow images of all three events, there are clear southward-moving structures. Events 1 and 2 are a single pulse with horizontal scales of ∼500–1,000 km. Event 3 shows five wave fronts with a horizontal scale size of 500–1,000 km. All three TIDs are medium-scale TIDs. Horizontal wavelengths of both airglow intensity at an average emission altitude of 250 km and CHAMP neutral density variations measured at 400 km are estimated by fitting a sinusoidal function to the observed data. The estimated horizontal wavelengths for airglow and neutral density data are 1,031 and 880 km for event 1 and 560 and 420 km for event 3, respectively. These values between airglow and CHAMP are comparable, suggesting both instruments are observing the same wave. For event 1, the CHAMP electron density mapped along the geomagnetic field line onto the airglow altitude does not show wave structure similar to the airglow variation. For events 2 and 3, the plasma density did not show wavy structures similar to the waves seen in the airglow image and CHAMP neutral density. These results suggest that the TIDs observed in airglow images are not caused by ionospheric plasma instability but by gravity waves in the thermosphere.
AB - We report the first comparison of ground and satellite measurements of low-latitude traveling ionospheric disturbances (TIDs). Three TID events were simultaneously observed by a 630.0-nm airglow imager and the CHAllenging Minisatellite Payload (CHAMP) satellite at Kototabang, Indonesia (geographic coordinates: 0.2° S, 100.3° E, geomagnetic latitude: 10.6° S). In 630.0-nm airglow images of all three events, there are clear southward-moving structures. Events 1 and 2 are a single pulse with horizontal scales of ∼500–1,000 km. Event 3 shows five wave fronts with a horizontal scale size of 500–1,000 km. All three TIDs are medium-scale TIDs. Horizontal wavelengths of both airglow intensity at an average emission altitude of 250 km and CHAMP neutral density variations measured at 400 km are estimated by fitting a sinusoidal function to the observed data. The estimated horizontal wavelengths for airglow and neutral density data are 1,031 and 880 km for event 1 and 560 and 420 km for event 3, respectively. These values between airglow and CHAMP are comparable, suggesting both instruments are observing the same wave. For event 1, the CHAMP electron density mapped along the geomagnetic field line onto the airglow altitude does not show wave structure similar to the airglow variation. For events 2 and 3, the plasma density did not show wavy structures similar to the waves seen in the airglow image and CHAMP neutral density. These results suggest that the TIDs observed in airglow images are not caused by ionospheric plasma instability but by gravity waves in the thermosphere.
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U2 - 10.1029/2018JA025634
DO - 10.1029/2018JA025634
M3 - Article
AN - SCOPUS:85063285913
SN - 2169-9380
VL - 124
SP - 2198
EP - 2212
JO - Journal of Geophysical Research: Space Physics
JF - Journal of Geophysical Research: Space Physics
IS - 3
ER -