Spectral and spatial images obtained with the Imaging Spectrometric Ob
servatory on the ATLAS 1 and Spacelab 1 missions are used to study the
ultraviolet emissions of nitric oxide in the thermosphere. By synthet
ically fitting the measured NO gamma bands, intensities are derived as
a function of altitude and latitude. We find that the NO concentratio
ns inferred from the ATLAS 1 measurements are higher than predicted by
our thermospheric airglow model and tend to lie to the high side of a
number of earlier measurements. By comparison with synthetic spectral
fits, the shape of the NO gamma bands is used to derive temperature a
s a function of altitude. Using the simultaneous spectral and spatial
imaging capability of the instrument, we present the first simultaneou
sly acquired altitude images of NP gamma band temperature and intensit
y in the thermosphere. The lower thermospheric temperature images show
structure as a function of altitude. The spatial imaging technique ap
pears to be a viable means of obtaining temperatures in the middle and
lower thermosphere, provided that good information is also obtained a
t the higher altitudes, as the contribution of the overlying, hotter N
O is nonnegligible. By fitting both self-absorbed and nonabsorbed band
s of the NO gamma system, we show that the self absorption effects are
observable up to 200 km, although small above 150 km. The spectral re
solution of the instrument (1.6 Angstrom) allows separation of the N+(
S-5) doublet, and we show the contribution of this feature to the comb
ination of the NO gamma (1,0) band and the N+(S-5) doublet as a functi
on of altitude (less than 10% below 200 km). Spectral images including
the NO delta bands support previous findings that the fluorescence ef
ficiency is much higher than that determined from laboratory measureme
nts, The Spacelab 1 data indicate the presence of a significant popula
tion of hot NO in the vehicle environment of that early shuttle missio
n.