The chemistry–climate model ECHAM6.3-HAM2.3-MOZ1.0
The chemistry–climate model ECHAM-HAMMOZ contains a detailed representation of tropospheric and stratospheric reactive chemistry and state-of-the-art parameterizations of aerosols using either a modal scheme (M7) or a bin scheme (SALSA). This article describes and evaluates the model version ECHAM6....
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Veröffentlicht in: | Geoscientific Model Development 2018-05, Vol.11 (5), p.1695-1723 |
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Hauptverfasser: | , , , , , , , , , , , , , , , , , , , , |
Format: | Artikel |
Sprache: | eng |
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Zusammenfassung: | The chemistry–climate model ECHAM-HAMMOZ contains a detailed representation
of tropospheric and stratospheric reactive chemistry and state-of-the-art
parameterizations of aerosols using either a modal scheme (M7) or a bin
scheme (SALSA). This article describes and evaluates the model version
ECHAM6.3-HAM2.3-MOZ1.0 with a focus on the tropospheric gas-phase chemistry.
A 10-year model simulation was performed to test the stability of the model
and provide data for its evaluation. The comparison to observations
concentrates on the year 2008 and includes total column observations of ozone
and CO from IASI and OMI, Aura MLS observations of temperature, HNO3,
ClO, and O3 for the evaluation of polar stratospheric
processes, an ozonesonde climatology, surface ozone observations from the
TOAR database, and surface CO data from the Global Atmosphere Watch network.
Global budgets of ozone, OH, NOx, aerosols, clouds, and radiation
are analyzed and compared to the literature. ECHAM-HAMMOZ performs well in
many aspects. However, in the base simulation, lightning NOx
emissions are very low, and the impact of the heterogeneous reaction of
HNO3 on dust and sea salt aerosol is too strong. Sensitivity
simulations with increased lightning NOx or modified heterogeneous
chemistry deteriorate the comparison with observations and yield excessively
large ozone budget terms and too much OH. We hypothesize that this is an
impact of potential issues with tropical convection in the ECHAM model. |
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ISSN: | 1991-9603 1991-959X 1991-962X 1991-9603 1991-962X |
DOI: | 10.5194/gmd-11-1695-2018 |