Jh. Yee et al., GLOBAL SIMULATIONS AND OBSERVATIONS OF O(S-1), O-2((1)SIGMA) AND OH MESOSPHERIC NIGHTGLOW EMISSIONS, J GEO R-S P, 102(A9), 1997, pp. 19949-19968
Despite a large number of observations of mesospheric nightglow emissi
ons in the past, the quantitative comparison between theoretical and e
xperimental brightnesses is rather poor, owing primarily to the short
duration of the observations, the strong variability of the tides, and
the influence of short-timescale gravity waves. The high-resolution D
oppler imager (HRDI) instrument onboard the upper atmosphere research
satellite (UARS) provides nearly simultaneous, near-global observation
s of O(S-1) green line, O-2(0-1) atmospheric band, and OH Meinel band
nightglow emissions. Three days of these observations near the Septemb
er equinox of 1993 are presented to show the general characteristics b
f the three emissions, including the emission brightness, peak emissio
n altitude, and their temporal and spatial variabilities. The global d
istribution of these emissions is simulated on the basis of atmospheri
c parameters from the recently developed National Center for Atmospher
ic Research (NCAR) thermosphere-ionosphere-mesospher-electrodynamics g
eneral circulation model (TIME-GCM). The most striking features reveal
ed by the global simulation are the structuring of the mesospheric nig
htglow by the diurnal tides and enhancements of the airglow at high la
titudes. The model reproduces the inverse relationship observed by HRD
I between the nightglow brightness and peak emission altitude. Analysi
s of our model results shows that the large-scale latitudinal/tidal ni
ghtglow brightness variations are a direct result df a complex interpl
ay between mesospheric and lower thermospheric diffusive and advective
processes, acting mainly on the atomic oxygen concentrations. The inc
lination of the UARS spacecraft precluded observations of high latitud
e nightglow emissions by HRDI. However,our predicted high-latitude bri
ghtness enhancements confirm previous limited groundbased observations
in the polar region. This work provides an initial validation of the
NCAR-TIMEGCM using airglow data.