Abstract
First results are presented from the conjugate maneuvers performed by NASA's Ionospheric Connection Explorer (ICON) spacecraft. During each several-minute maneuver, ICON crosses the magnetic equator, measuring the plasma drift at the ∼600-km apex of a magnetic field line and the neutral wind profiles (∼90–300 km altitude) along both ends of that field line. The analysis utilizes 149 pairs of maneuvers separated by ∼24 hr but at nearly the same location and local time. Principal component regression reveals that 39 ± 7% and 24 ± 9% of the day-to-day variance in the daytime vertical and zonal drift, respectively, is attributable to conjugate neutral winds. The remaining variance is likely driven by external potentials from non-conjugate winds and geomagnetic activity (median Kp 2−). Zonal winds at 100–113 km and >120 km altitude are the primary drivers of conjugate vertical and zonal drift variance, respectively. These observations can test vertical-coupling mechanisms in whole-atmosphere models.
Original language | English (US) |
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Article number | e2023GL107110 |
Journal | Geophysical Research Letters |
Volume | 51 |
Issue number | 5 |
DOIs | |
State | Published - Mar 16 2024 |
Keywords
- ICON
- electric fields
- ionosphere-thermosphere coupling
- ionospheric variability
- neutral wind dynamo
- vertical coupling
ASJC Scopus subject areas
- Geophysics
- General Earth and Planetary Sciences