HR: 0800h
AN: SA31A-12 [Abstracts]
TI: Mesospheric Gravity wave momentum fluxes and their seasonal variation over a low latitude region Trivandrum (8.5°N, 77°E), India
AU: * Antonita, M
EM: mariaspl@gmail.com
AF: Space Physics Laboratory, Vikram Sarabhai Space Center,Trivandrum – 695022 ,India,
Space Physics Laboratory, Vikram Sarabhai Space Center,Trivandrum – 695022 ,India, Trivandrum, 695022,
India
AU: Ramkumar, G
EM: geetha_ramkumar@vssc.gov.in
AF: Space Physics Laboratory, Vikram Sarabhai Space Center,Trivandrum – 695022 ,India,
Space Physics Laboratory, Vikram Sarabhai Space Center,Trivandrum – 695022 ,India, Trivandrum, 695022,
India
AU: Kishore Kumar, K
EM: kishore_nmrf@yahoo.com
AF: Space Physics Laboratory, Vikram Sarabhai Space Center,Trivandrum – 695022 ,India,
Space Physics Laboratory, Vikram Sarabhai Space Center,Trivandrum – 695022 ,India, Trivandrum, 695022,
India
AB:
Gravity waves play a profound role in the energetics and dynamics of the MLT region. Mainly generated in the
lower atmosphere they propagate vertically upwards, thus carrying energy and momentum fluxes from lower
atmosphere to MLT region where they attain maximum wave amplitudes. Determining the gravity wave
momentum fluxes is a crucial requirement in understanding the momentum and energy budgets of the MLT
region. Earlier studies have been carried out using VHF and MF radars, which have limited seasonal and height
coverage. To understand the global morphology of gravity wave momentum fluxes, continuous measurements of
winds are required in MLT region. Meteor wind radars are well suited for this purpose owing to their uninterrupted
data coverage. Using two years of data (2004-2006) from All-sky SKiYMET Meteor Wind Radar at Space Physics
Laboratory (SPL), Trivandrum (8.5°N, 77°E) operating at a VHF frequency of 35.25 MHz and a pulse
repetition frequency of 2144 Hz, an attempt has been made to estimate the momentum fluxes of gravity waves in
the MLT region (82-98km). Seasonal variation in the momentum fluxes is also estimated. The detailed study will
be presented.
DE: 1620 Climate dynamics (0429, 3309)
DE: 3332 Mesospheric dynamics
DE: 3334 Middle atmosphere dynamics (0341, 0342)
SC: SPA-Aeronomy [SA]
MN: 2007 Joint Assembly