Hg. Mayr et al., THE GRAVITY-WAVE DOPPLER SPREAD THEORY APPLIED IN NUMERICAL SPECTRAL MODEL OF THE MIDDLE ATMOSPHERE .1. MODEL AND GLOBAL-SCALE SEASONAL-VARIATIONS, J GEO RES-A, 102(D22), 1997, pp. 26077-26091
Hines [1997a, b] has developed a Doppler spread parameterization (DSP)
for the deposition of small-scale gravity wave (GW) momentum and ener
gy in the middle atmosphere. We have incorporated this DSP into the tw
o-dimensional (2-D) version of the numerical spectral model (NSM) of C
hart et al. [1994a, b] which is applied to the Earth's middle atmosphe
re. With a globally uniform flux of(quasi) isotropically propagating G
W emanating from the troposphere, the NSM has been integrated for seve
ral model years to describe seasonal variations and equatorial oscilla
tions. Here, after a review of the NSM and DSP, we discuss numerical r
esults that describe the temperature and wind fields during solstice a
nd equinox conditions, emphasizing the role played by the GW spectrum.
That spectrum is filtered as it ascends through the stratosphere and
provides, at the solstices, a highly anisotropic wave and momentum flu
x at mesospheric heights. Upon further filtering there, with attendant
momentum deposition, the waves decelerate and then reverse the zonal
circulation. In quasi-geostrophic balance latitudinally, this reversal
is accompanied by a reversal of the latitudinal temperature gradient,
one that leads to a temperature minimum in the summer polar mesopause
region, as is observed. Corresponding results for equinox are obtaine
d, and all are discussed. Our results differ only in detail from those
of similar analyses that employ other GW parameterizations. They are
presented here in part to exhibit the success of the DSP at this eleme
ntary level and in part to provide a point of departure against which
future refinements may be judged. Our first extension of the modeling
concerns the semiannual and quasi-biennial oscillations that are produ
ced by the DSP in the NSM at equatorial latitudes with the same, const
ant and uniform, incident GW flux. Initial results are presented in th
e companion paper and are compared there with observations.