Longitude variability of the solar semidiurnal tide in the lower thermosphere through assimilation of ground- and space-based wind measurements

Physics – Space Physics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

13

Meteorology And Atmospheric Dynamics: Waves And Tides, Meteorology And Atmospheric Dynamics: Thermospheric Dynamics (0358), Atmospheric Composition And Structure: Instruments And Techniques, Meteorology And Atmospheric Dynamics: Instruments And Techniques

Scientific paper

Wind measurements from the Upper Atmosphere Research Satellite (UARS) and model output from the Middle Atmosphere General Circulation Model (GCM) at Kyushu University are used to investigate the nature of nonmigrating semidiurnal tides between 50-55°N using combined space-based (SBM) and ground-based (GBM) wind measurements at 95 km. The GCM is used to create a mock database to test the effects of various sampling scenarios, data gaps, and relative weighting between SBM and GBM, on retrieval of the longitude structure of the semidiurnal tide. SB sampling is based upon orbital characteristics of UARS. GB sampling corresponds to hourly radar measurements from Saskatoon (52°N, 107°W), Sheffield (53°N, 4°W), Collm (52°N, 15°E), Obninsk (55°N, 37°E), and Kazan (56°N, 49°E). Results are presented for the month of August when semidiurnal amplitudes are large and sampling by UARS instruments is good. By compositing over a 5-10 day ``fit span,'' it is found that the combination of temporal coverage by GB radars and spatial sampling by the satellite is sufficient to allow reasonable recovery of the zonal wave number s = 1, 2, 3 components of the semidiurnal tide. Over significantly longer fit spans, the contributions of GBM become less critical. Using actual UARS and GBM during 1-20 August 1993, the semidiurnal amplitude of eastward wind is found to vary from a minimum value (12 ms-1) at 20°E, to a maximum of 45 ms-1 near 160°E, and a secondary maximum (29 ms-1) at 300°E. The zonal wave number components corresponding to this longitude variation in the semidiurnal tide are 7.7 +/- 1.9 ms-1, 19.8 +/- 1.5 ms-1 and 13.0 +/- 1.3 ms-1 for s = 1, 2, 3 (westward), respectively where +/-1-σ uncertainties are indicated. These results are in reasonable agreement with those simulated within the Kyushu GCM. However, there is roughly a four- to five-hour phase offset between the phases recovered from the observational data and from the Kyushu GCM, possibly connected with strong model phase gradients in this atmospheric regime.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Longitude variability of the solar semidiurnal tide in the lower thermosphere through assimilation of ground- and space-based wind measurements does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Longitude variability of the solar semidiurnal tide in the lower thermosphere through assimilation of ground- and space-based wind measurements, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Longitude variability of the solar semidiurnal tide in the lower thermosphere through assimilation of ground- and space-based wind measurements will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1463289

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.