Internal gravity waves in the thermosphere during low and high solar activity: Simulation study

Details Internal gravity waves in the thermosphere during low and high solar activity: Simulation study Internal gravity waves in the thermosphere during low and high solar activity: Simulation study

Aug 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010jgra..11500g02y&link_type=abstract

Journal of Geophysical Research, Volume 115, Issue A2, CiteID A00G02

Physics

3

Atmospheric Processes: Thermospheric Dynamics (0358), Oceanography: Physical: Internal And Inertial Waves, Ionosphere: Wave Propagation (0689, 3285, 4275, 4455, 6934), Atmospheric Processes: General Circulation (1223), Space Weather: Solar Effects

Scientific paper

Propagation of internal gravity waves (GWs) from the lower atmosphere into the upper thermosphere, and their dynamical and thermal effects have been studied under low and high solar activity approximated by the F10.7 parameter. It has been done by using a nonlinear spectral parameterization in systematic offline calculations with typical wind and temperature distributions from the HWM and MSISE-90 models, and with interactive simulations using the University College London Coupled Middle Atmosphere-Thermosphere-2 (CMAT2) general circulation model (GCM) under solstice conditions. The estimates have been performed for relatively slow harmonics with horizontal phase velocities less than 100 m s-1, which are not affected by reflection and/or ducting. GW drag and wave-induced heating/cooling are shown to be smaller below ˜170 km at high solar activity, and larger above. The maxima of GW momentum deposition occur much higher in the upper thermosphere, but their peaks are half as strong, 120 vs 240 m s-1 day-1 in the winter hemisphere when the insolation is large. Instead of strong net cooling in the upper thermosphere, GWs produce a weak heating at high solar activity created by fast harmonics less affected by dissipation. Molecular viscosity increases with solar activity at fixed pressure levels, but seen in Cartesian altitude grids it can either increase or decrease in the lower thermosphere, depending on the height. Therefore, in pressure coordinates, in which most GCMs operate, the influence of larger temperatures can be viewed as a competition between the enhanced dissipation and vertical expansion of the atmosphere.

Affiliated with

Also associated with

No associations

Rating

Internal gravity waves in the thermosphere during low and high solar activity: Simulation study 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 Internal gravity waves in the thermosphere during low and high solar activity: Simulation study, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Internal gravity waves in the thermosphere during low and high solar activity: Simulation study will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-981481