Physically based modeling of atmosphere-to-snow-to-firn transfer of H₂O₂ at South Pole

dc.contributor.authorMcConnell, Joseph R.
dc.contributor.authorBales, Roger C.
dc.contributor.authorStewart, Richard W.
dc.contributor.authorThompson, Anne M.
dc.contributor.authorAlbert, Mary R.
dc.contributor.authorRamos, Ricardo
dc.date.accessioned2024-07-26T16:34:06Z
dc.date.available2024-07-26T16:34:06Z
dc.date.issued1998-05-01
dc.description.abstractQuantitative interpretation of ice core chemical records requires a detailed understanding of the transfer processes that relate atmospheric concentrations to those in the snow, firn, and ice. A unique, 2 year set of year-round surface snow samples at South Pole and snow pits, with associated accumulation histories, were used to test a physically based model for atmosphere-to-firn transfer of H₂O₂. The model, which extends our previous transfer modeling at South Pole into the snowpack, is based on the advection-dispersion equation and spherical diffusion within representative snow grains. Required physical characteristics of the snowpack, such as snow temperature and ventilation, were estimated independently using established physical models. The surface snow samples and related model simulations show that there is a repeatable annual cycle in H₂O₂ in the surface snow at South Pole. It peaks in early spring, and surface snow concentration is primarily determined by atmospheric concentration and temperature, with some dependence on grain size. The snow pits and associated model simulations point out the importance of accumulation timing and annual accumulation rate in understanding the deposition and preservation of H₂O₂ and δ¹⁸O at South Pole. Long-term snowpack simulations suggest that the firn continues to lose H₂O₂ to the atmosphere for at least 10–12 years (~3 m) after burial at current South Pole temperatures and accumulation rates.
dc.description.sponsorshipThis work was supported by a NASA Graduate Fellowship for Global Change and in part by National Science Foundation's Office of Polar Program. Atmospheric photo chemical modeling at NASA was sup-ported by the Goddard Director's Discretionary Fund. Fieldwork at South Pole was conducted under a cooperative agreement with the NOAA Climate Monitoring and Diagnostics Laboratory (CMDL). We very much appreciate the efforts of K. McNitt, M. Boland, J. Otten, B. Halter, and T. Swanson of NOAA/CMDL for their help at South Pole and S. Oltmans and P. Novelli for access to the surface ozone and carbon monoxide data, respectively. We also thank A.Long and D. Dettman for access to the University of Arizona stable isotope lab and B. Snider for her help with laboratory measurements.
dc.description.urihttps://agupubs.onlinelibrary.wiley.com/doi/abs/10.1029/98JD00460
dc.format.extent10 pages
dc.genrejournal articles
dc.identifierdoi:10.13016/m2f3hi-ux5m
dc.identifier.citationMcConnell, Joseph R., Roger C. Bales, Richard W. Stewart, Anne M. Thompson, Mary R. Albert, and Ricardo Ramos. “Physically Based Modeling of Atmosphere-to-Snow-to-Firn Transfer of H₂O₂ at South Pole.” Journal of Geophysical Research: Atmospheres 103, no. D9 (1998): 10561–70. https://doi.org/10.1029/98JD00460.
dc.identifier.urihttps://doi.org/10.1029/98JD00460
dc.identifier.urihttp://hdl.handle.net/11603/34918
dc.language.isoen_US
dc.publisherAGU
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC GESTAR II
dc.rightsThis work was written as part of one of the author's official duties as an Employee of the United States Government and is therefore a work of the United States Government. In accordance with 17 U.S.C. 105, no copyright protection is available for such works under U.S. Law.
dc.rightsPublic Domain
dc.rights.urihttps://creativecommons.org/publicdomain/mark/1.0/
dc.titlePhysically based modeling of atmosphere-to-snow-to-firn transfer of H₂O₂ at South Pole
dc.typeText
dcterms.creatorhttps://orcid.org/0000-0002-7829-0920

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