Influence of model resolution of model resolution on the atmospheric transport of Be-10

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dc.contributor.authorHeikkilä, UEen_AU
dc.contributor.authorSmith, AMen_AU
dc.date.accessioned2014-03-31T22:58:01Zen_AU
dc.date.available2014-03-31T22:58:01Zen_AU
dc.date.issued2012-01-01en_AU
dc.date.statistics2014-04-01en_AU
dc.description.abstractUnderstanding the transport path of the solar activity proxy Be-10 from source to archive is crucial for the interpretation of its observed variability. The extent of mixing of the strong production signal has been quantified in a previous study (Heikkila et al., 2009). In this study we perform sensitivity studies to investigate the influence of model resolution on the degree of mixing and transport path of Be-10 in the atmosphere using the ECHAM5-HAM aerosol-climate model. This study permits us to choose an acceptable resolution, and so minimum CPU time, to produce reconstructions as physically accurate as possible. Five model resolutions are applied: T21L19: a coarse horizontal and vertical resolution with model top at ca. 30 km, T42L31: an average horizontal and fine vertical one, T42L39: similar vertical resolution than L19 but including the middle atmosphere up to ca. 80 km, T63L31: a fine horizontal and vertical resolution and T63L47: a fine resolution horizontally and vertically with middle atmosphere. Comparison with observations suggests that a finer horizontal and vertical resolution might be beneficial, producing a reduced meridional gradient, although the spread between observations was much larger than between the five model runs. In terms of atmospheric mixing the differences became more distinguishable. All resolutions agreed that the main driver of deposition variability, observed in natural archives, is the input of stratospheric Be-10 (total contribution 68 %) which is transported into the troposphere at latitudes 30-50 degrees. In the troposphere the model resolutions deviated largely in the dispersion of the stratospheric component over latitude. The finest resolution (T63L47) predicted the least dispersion towards low latitudes but the most towards the poles, whereas the coarsest resolution (T21L19) suggested the opposite. The tropospheric components of Be-10 differed less between the five model runs. The largest differences were found in the polar tropospheric components, which contribute the least to total production (approximate to 4 %). We conclude that the use of the T42 horizontal resolution seems to be sufficient in terms of atmospheric mixing of a stratospheric tracer because no substantial improvement was seen when the resolution was increased from T42 to T63. The use of the middle atmospheric configuration is a trade-off between correctly describing stratospheric dynamics and having to reduce vertical resolution. The use of a high vertical resolution seemed more beneficial than the middle atmospheric configuration in this study. The differences found between the T42L31 and T63L31 resolutions were so small that T42L31 is a good choice because of its computational efficiency. © Author(s) 2012.en_AU
dc.identifier.citationHeikkilä, U., & Smith, A. M. (2012). Influence of model resolution of model resolution on the atmospheric transport of Be-10. Atmospheric Chemistry and Physics, 12(21), 10601-10612. doi:10.5194/acp-12-10601-2012en_AU
dc.identifier.govdoc4652en_AU
dc.identifier.issn1680-7316en_AU
dc.identifier.issue21en_AU
dc.identifier.journaltitleAtmospheric Chemistry and Physicsen_AU
dc.identifier.pagination10601-10612en_AU
dc.identifier.urihttp://dx.doi.org/10.5194/acp-12-10601-2012en_AU
dc.identifier.urihttp://apo.ansto.gov.au/dspace/handle/10238/5363en_AU
dc.identifier.volume12en_AU
dc.language.isoenen_AU
dc.publisherCopernicus Gesellschaft MBHen_AU
dc.subjectResolutionen_AU
dc.subjectSolar activityen_AU
dc.subjectClimate modelsen_AU
dc.subjectSensitivityen_AU
dc.subjectDepositionen_AU
dc.subjectAiren_AU
dc.titleInfluence of model resolution of model resolution on the atmospheric transport of Be-10en_AU
dc.typeJournal Articleen_AU
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