Abstract
We report for the first time the day-to-day variation of the longitudinal structure in height of the F2 layer (hmF2) in the equatorial ionosphere using multi-satellite observations of electron density profiles by the Constellation Observing System for Meteorology, Ionosphere and Climate-2 (COSMIC-2). These observations reveal a ∼3-day modulation of the hmF2 wavenumber-4 structure viewed in a fixed local time frame during January 30–February 14, 2021. Simultaneously, ∼3-day planetary wave activity is discerned from zonal wind observations at ∼100 km by the Ionospheric Connection Explorer (ICON) Michelson Interferometer for Global High-Resolution Thermospheric Imaging (MIGHTI). This signature is not observed at ∼180–250 km altitudes, suggesting the dissipation of this wave below the F-region. We propose that the 3-day variation identified in hmF2 is likely caused by the planetary wave-tide interaction through the E-region dynamo.
| Original language | English |
|---|---|
| Article number | e2021GL094877 |
| Journal | Geophysical Research Letters |
| Volume | 48 |
| Issue number | 15 |
| DOIs | |
| State | Published - Aug 2021 |
Keywords
- equatorial ionosphere
- ion neutral connection
- planetary waves
- tides
- upper atmosphere
- wave interaction