This study presents multi-instrument observations of persistent large-scale traveling ionosphere/atmospheric disturbances (LSTIDs/LSTADs) observed during moderately increased auroral electrojet activity and a sudden stratospheric warming in the polar winter hemisphere. The Global Ultraviolet Imager (GUVI), Gravity field and steady-state Ocean Circulation Explorer, Scanning Doppler Imaging Fabry–Perot Interferometers, and the Poker Flat Incoherent Scatter Radar are used to demonstrate the presence of LSTIDs/LSTADs between 19 UT and 5 UT on 18–19 January 2013 over the Alaska region down to lower midlatitudes. This study showcases the first use of GUVI for the study of LSTADs. These novel GUVI observations demonstrate the potential for the GUVI far ultraviolet emissions to be used for global-scale studies of waves and atmospheric disturbances in the thermosphere, a region lacking in long-term global measurements. These observations typify changes in the radiance from around 140 to 180 km, opening a new window into the behavior of the thermosphere.
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This content will become publicly available on February 1, 2027
Poleward Disturbances in Thermospheric Winds During the 3–4 November 2021 Geomagnetic Storm
Abstract This study focuses on ionosphere‐thermosphere coupling over North America during the 3–4 November 2021 strong geomagnetic storm (Kp 8−). We comprehensively analyze storm‐time ionospheric and thermospheric disturbances using data from ground‐based instruments at Poker Flat, Millstone Hill, and Urbana, as well as satellite observations and model data. Significant features of ionosphere‐thermosphere dynamics during the storm include (a) equatorward (−300 m/s) and poleward (50 m/s) surges at Millstone Hill (42.37 glat) and a poleward surge (75 m/s) at Urbana (40.13 glat) in the magnetic local time (MLT) post‐midnight sector, (b) ion velocities greater than −1,500 m/s at Poker Flat accompanied by a deep ionospheric trough moving to latitudes as low as 40 glat suggesting SAPS activity, (c) a widespread electron density depression in the morning hours due to an extended composition disturbance zone and (d) Large‐Scale Traveling Ionospheric Disturbances (LSTIDs) related to disturbances in equatorward winds in the post‐poleward wind interval. Results show that the equatorward and poleward surges were not accompanied by LSTIDs, which suggests that the extreme disturbances in meridional winds could have mainly been caused by SAPS forcing, due to ion drag and pressure gradients, rather than equatorward propagating Traveling Atmospheric Disturbances (TADs). Furthermore, the MLT location of Millstone Hill and Urbana indicates that during the disturbances both stations would have been located within the eastward backflow sector of the SAPS, which likely contributed to the complicated ion‐neutral dynamics.
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- Award ID(s):
- 2431743
- PAR ID:
- 10672304
- Publisher / Repository:
- AGU JGR Space Physics
- Date Published:
- Journal Name:
- Journal of Geophysical Research: Space Physics
- Volume:
- 131
- Issue:
- 2
- ISSN:
- 2169-9380
- Format(s):
- Medium: X
- Sponsoring Org:
- National Science Foundation
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