Abstract
We present direct observations of the semidiurnal lunar tide zonal winds at 260km and 350km during low solar activity in 2007-2008, and 2010-2011. The migrating semidiurnal lunar tide, or M2, is a global feature with amplitudes of about 10ms-1 at equatorial latitudes, and 20ms-1 at high latitudes. Amplitude maxima appear twice yearly, between February and April and between August and November. M2 amplitudes during 2007-2008 are about 20% stronger than those during 2010-2011. These magnitudes are consistent with numerical predictions in WACCM-X. However, only one annual global-scale maximum is simulated during January-March.
| Original language | English |
|---|---|
| Pages (from-to) | 126-133 |
| Number of pages | 8 |
| Journal | Journal of Atmospheric and Solar-Terrestrial Physics |
| Volume | 136 |
| DOIs | |
| State | Published - Dec 1 2015 |
Keywords
- Lunar
- Semidiurnal
- Thermosphere
- Tide