Abstract. We use data from two NASA satellites, the Thermosphere Ionosphere Energetics
and Dynamics (TIMED) and the Aeronomy of Ice in the Mesosphere (AIM)
satellites, in conjunction with model simulations from the
thermosphere-ionosphere-mesosphere-electrodynamics general circulation model
(TIME-GCM) to elucidate the key dynamical and chemical factors governing the
abundance and diurnal variation of lower thermospheric nitric
oxide (NO) at near-solar minimum conditions and low latitudes. This analysis
was enabled by the recent orbital precession of the AIM satellite which
caused the solar occultation pattern measured by the Solar Occultation for
Ice Experiment (SOFIE) to migrate down to low and mid-latitudes for specific
periods of time. We use a month of NO data collected in January 2017
to compare with two versions of the TIME-GCM; one is driven solely by
climatological tides and analysis-derived planetary waves at the lower
boundary and is free running at all other altitudes, and the other is
constrained by a high-altitude analysis from the Navy Global Environmental
Model (NAVGEM) up to the mesopause. We also compare SOFIE data with a
NO climatology from the nitric oxide empirical model (NOEM). Both
SOFIE and NOEM yield peak NO abundances of around 4×107 cm−3; however, the SOFIE profile peaks about 6–8 km lower than
NOEM. We show that this difference is likely a local time effect, with SOFIE
being a dawn measurement and NOEM representing late morning and/or near noon.
The constrained version of TIME-GCM exhibits a low-altitude dawn peak, while
the model that is forced solely at the lower boundary and free
running above does not. We attribute this difference to a phase change in the
semi-diurnal tide in the NAVGEM-constrained model, causing the descent of
high NO mixing ratio air near dawn. This phase difference between the
two models arises due to differences in the mesospheric zonal mean zonal
winds. Regarding the absolute NO abundance, all versions of the
TIME-GCM overestimate this. Tuning the model to yield calculated atomic
oxygen in agreement with TIMED data helps but is insufficient. Furthermore,
the TIME-GCM underestimates the electron density (Ne) as compared with the
International Reference Ionosphere (IRI) empirical model. This suggests a
potential conflict with the requirements of NO modeling and Ne
modeling, since one solution typically used to increase model Ne is to
increase the solar soft X-ray flux, which would, in this case, worsen the
NO model–data discrepancy.