Mathematics – Logic
Scientific paper
Sep 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989maph...29...86k&link_type=abstract
In International Council of Scientific Unions, Middle Atmosphere Program. Handbook for MAP, Volume 29. Part 1: Extended Abstract
Mathematics
Logic
Atmospheric Heating, Ozone, Planetary Waves, Short Wave Radiation, Solar Rotation, Boundary Conditions, Excitation, Geopotential, Resonance, Solar Oscillations, Solar Wind, Stratosphere, Troposphere
Scientific paper
It is known that there are variations in the atmospheric processes with a period close to that of the rotation of the Sun (27 days). The variations are discovered in tropospheric processes, rainfalls, geopotential and in stratosphere. The main theoretical problem is the identification of the physical process by which these heterogeneous solar and meteorological phenomena are connected. Ivanovsky and Krivolutsky proposed that the periodic heating of the ozone layer by the short wave radiation would be the reason of excitation the 27-day oscillations. It was also assumed that excitement takes place in condition of resonance with an excited mode corresponding to the conditions present in the stratospheric circulations. The possibility is discussed of the resonant excitation and presentation is made of the data analysis results which support this idea.
No associations
LandOfFree
Atmospheric planetary waves induced by solar rotation 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 Atmospheric planetary waves induced by solar rotation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Atmospheric planetary waves induced by solar rotation will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-766067