Physics
Scientific paper
Feb 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006jastp..68..309h&link_type=abstract
Journal of Atmospheric and Solar-Terrestrial Physics, Volume 68, Issue 3-5, p. 309-316.
Physics
Scientific paper
Kinetic energy dissipation rates for the auroral MLT have been obtained from the Tromsø middle frequency radar (MFR) and compared with simultaneous measurements of neutral wind-shears obtained from the Nippon/Norway Tromsø meteor radar (NTMR). Since wind-shears can drive dynamic instabilities which in turn result in turbulent dissipation of kinetic energy, we would expect these parameters to be correlated, and this is indeed the case. Having established this correlation we quantitatively combine the results from each radar to estimate the turbulent diffusion coefficient for momentum; considering the tentative nature of this approach, we find the agreement with previous estimates to be surprisingly good.
Aso Takehiko
Hall Chris Michael
Manson Alan H.
Meek Chris E.
Nozawa Satoshi
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