G. Pitari et E. Mancini, Climatic impact of future supersonic aircraft: Role of water vapour and ozone feedback on circulation, PHYS CH P C, 26(8), 2001, pp. 571-576
Citations number
18
Categorie Soggetti
Earth Sciences
Journal title
PHYSICS AND CHEMISTRY OF THE EARTH PART C-SOLAR-TERRESTIAL AND PLANETARY SCIENCE
Assessment studies of future supersonic aircraft impact on the chemical com
position of the atmosphere have generally been made using two- or three-dim
ensional chemical transport models (CTM). Typical products of these calcula
tion are ozone profile and column changes produced by NOx, H2O and particle
emissions from supersonic aircraft (HSCT). These have to be interpreted as
pure chemical perturbations, being the atmospheric circulation kept fixed
in the models. On the other hand, steady state accumulation of H2O from HSC
T can produce significant anomalies in the lower stratospheric water vapour
mixing ratio (about 10% at Northern mid-latitudes). Stratospheric H2O and
O-3 absorb longwave planetary radiation, so that HSCT driven changes may up
set the residual circulation and produce a radiative forcing at the tropopa
use. A climate-chemistry model is used here to study this effect, using an
iterative procedure for the chemistry and radiation modules that are not si
multaneously interactive. The major findings are the following: (a) lower s
tratospheric vertical fluxes of H2O and other atmospheric tracers are signi
ficantly affected by water vapour and ozone radiative feedback on the strat
ospheric circulation. (b) H2O accumulation patterns change significantly in
the tropical lower stratosphere, with respect to the case with no radiativ
e feedback on circulation of HSCT additional H2O and perturbed 03 (baseline
case). (c) The tropopause radiative forcing of this additional water vapou
r is greatly reduced with respect to the baseline case. (C) 2001 Elsevier S
cience Ltd. All rights reserved.