Physics
Scientific paper
Feb 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007cajph..85..153l&link_type=abstract
Canadian Journal of Physics, Vol. 85, No. 2, p. 153-172
Physics
Lower Thermosphere, Emission Rate, Waves, Mesosphere, Imager, Midlatitudes, Instrument, Radars
Scientific paper
Long-term ground-based airglow observations with a spectral airglow temperature imager (SATI) installed at Sierra Nevada Observatory (37.06 degrees N, 3.38 degrees W) at 2900 m height are used to investigate the main features of the quasi planetary waves in the period range of 3-20 days during autumn at this latitude in the mesosphere and lower thermosphere region. The modulations of periods 5 day, (6-7) day, and 10 day have been clearly detected during autumn at this location, being the most prominent waves detected at this location during the autumn. They have a strong persistence during the autumn period and relative amplitudes are generally constant during the period although a slight tendency to increase seems to be detected towards winter.
Aushev V. M.
Brown Shanique
Garcia-Comas Maya
Lopez-Gonzalez Maria José
Rodríguez Eduardo
No associations
LandOfFree
O-2 Atmospheric band and OH(6-2) airglow and temperature variability over Spain using SATI observations: Planetary-scale oscillations during autumn 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 O-2 Atmospheric band and OH(6-2) airglow and temperature variability over Spain using SATI observations: Planetary-scale oscillations during autumn, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and O-2 Atmospheric band and OH(6-2) airglow and temperature variability over Spain using SATI observations: Planetary-scale oscillations during autumn will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-736287