J. Schoendorf et al., NEUTRAL DENSITY CELLS IN THE HIGH-LATITUDE THERMOSPHERE .2. MECHANISMS, Journal of atmospheric and terrestrial physics, 58(15), 1996, pp. 1769-1781
NCAR-TIGCM simulations predict mesoscale cellular structures in the hi
gh Latitude neutral density at altitudes from 120-350 km. During magne
tically active conditions, the density structure at 200 km consists of
low-density cells near dawn and dusk and high-density cells near noon
and midnight. Mechanisms causing the structured density cells are a r
esult of thermosphere-ionosphere coupling and can be explained in term
s of dynamic meteorology. For example, at high latitudes ion drag caus
es the neutral circulation to flow cyclonically in the dawn sector and
anticyclonically in the dusk sector. Low densities are contained with
in the cyclonic circulation at all altitudes. Below about 170 km, the
densities inside the anticyclonic flow are high, while above that alti
tude densities within the anticyclonic flow are low. While typical dyn
amic meteorology explains low densities in the centre of cyclonic circ
ulation and high densities inside anticyclonic circulation, the dusk l
ow-density cell in the centre of anticyclonic how is unexpected. The a
nticyclonic dusk low-density cell is explained by anomalous antibaric
flow due to high-speed winds. 120 km and 200 km altitudes are used to
demonstrate the relationship between the high latitude densities and w
inds as well as the effect of joule heating and auroral particle preci
pitation on the density structures. Copyright (C) 1996 Elsevier Scienc
e Ltd