Abstract. Water vapour and ozone are important for the thermal and
radiative balance of the upper troposphere (UT) and lowermost stratosphere
(LMS). Both species are modulated by transport processes. Chemical and
microphysical processes affect them differently. Thus, representing the
different processes and their interactions is a challenging task for
dynamical cores, chemical modules and microphysical parameterisations of
state-of-the-art atmospheric model components. To test and improve the
models, high-resolution measurements of the UT–LMS are required. Here, we
use measurements taken in a flight of the GLORIA (Gimballed Limb Observer
for Radiance Imaging of the Atmosphere) instrument on HALO (High Altitude and LOng Range Research Aircraft). The German
research aircraft HALO performed a research flight on 26 February 2016 that covered deeply subsided
air masses of the aged 2015/16 Arctic vortex, high-latitude LMS air masses,
a highly textured region affected by troposphere-to-stratosphere exchange
and high-altitude cirrus clouds. Therefore, it provides a challenging
multifaceted case study for comparing GLORIA observations with
state-of-the-art atmospheric model simulations in a complex UT–LMS region at
a late stage of the Arctic winter 2015/16. Using GLORIA observations in this manifold scenario, we test the ability of
the numerical weather prediction (NWP) model ICON (ICOsahedral
Nonhydrostatic) with the extension ART (Aerosols and Reactive Trace gases)
and the chemistry–climate model (CCM) EMAC (ECHAM5/MESSy Atmospheric Chemistry – fifth-generation European Centre Hamburg general circulation model/Modular Earth Submodel System) to model the UT–LMS composition of water vapour (H2O), ozone
(O3), nitric acid (HNO3) and clouds. Within the scales resolved by
the respective model, we find good overall agreement of both models with
GLORIA. The applied high-resolution ICON-ART set-up involving an R2B7 nest
(local grid refinement with a horizontal resolution of about 20 km),
covering the HALO flight region, reproduces mesoscale dynamical structures
well. Narrow moist filaments in the LMS observed by GLORIA at tropopause
gradients in the context of a Rossby wave breaking event and in the vicinity of
an occluded Icelandic low are clearly reproduced by the model. Using
ICON-ART, we show that a larger filament in the west was transported
horizontally into the Arctic LMS in connection with a jet stream split
associated with poleward breaking of a cyclonically sheared Rossby wave.
Further weaker filaments are associated with an older tropopause fold in the
east. Given the lower resolution (T106) of the nudged simulation of the EMAC
model, we find that this model also reproduces these features well. Overall,
trace gas mixing ratios simulated by both models are in a realistic range,
and major cloud systems observed by GLORIA are mostly reproduced. However,
we find both models to be affected by a well-known systematic moist bias in
the LMS. Further biases are diagnosed in the ICON-ART O3, EMAC H2O
and EMAC HNO3 distributions. Finally, we use sensitivity simulations to
investigate (i) short-term cirrus cloud impacts on the H2O distribution
(ICON-ART), (ii) the overall impact of polar winter chemistry and
microphysical processing on O3 and HNO3 (ICON-ART and EMAC), (iii) the impact of the model resolution on simulated parameters (EMAC), and (iv) consequences of scavenging processes by cloud particles (EMAC). We find that
changing the horizontal model resolution results in notable systematic
changes for all species in the LMS, while scavenging processes play a role
only in the case of HNO3. We discuss the model biases and deficits found in
this case study that potentially affect forecasts and projections
(adversely) and provide suggestions for further model improvements.