An overview of ISCAT 2000

D. D. Davis, F. Eisele, G. Chen, J. Crawford, G. Huey, D. Tanner, D. Slusher, L. Mauldin, S. Oncley, D. Lenschow, S. Semmer, R. Shetter, B. Lefer, R. Arimoto, A. Hogan, P. Grube, M. Lazzara, A. Bandy, D. Thornton, H. BerresheimH. Bingemer, M. Hutterli, J. McConnell, R. Bales, J. Dibb, M. Buhr, J. Park, Peter H McMurry, A. Swanson, S. Meinardi, D. Blake

Research output: Contribution to journalArticlepeer-review

46 Scopus citations


The Investigation of Sulfur Chemistry in the Antarctic Troposphere (ISCAT) took place over the timer period of 15 November to 31 December in the year 2000. The study location was the Amundsen Scott Station in Antarctica. ISCAT 2000 defines the second phase of a program designed to explore tropospheric chemistry in Antarctica. As in 1998, the 2000 ISCAT study revealed a strong oxidizing environment at South Pole (SP). During the 2000 investigation, however, the suite of measurements was greatly expanded. These new measurements established the recycling of reactive nitrogen as a critical component of this unique environment. This paper first presents the historical background leading up to the ISCAT 2000 observations; then it focuses on providing a summary of the year 2000 results and contrasts these with those recorded during 1998. Important developments made during the 2000 study included the recording of SP data for several species being emitted from the snowpack. These included NO, H 2O2 and CH2O. In this context, eddy-diffusion flux measurements provided the first quantitative estimates of the SP NO and NOx snow-to-atmosphere fluxes. This study also revealed that HNO 3 and HO2NO2 were major sink species for HOx and NOx radicals. And, it identified the critical factors responsible for SP NO levels exceeding those at other polar sites by nearly an order of magnitude. Finally, it reports on the levels of gas phase sulfur species and provides evidence indicating that the absence of DMS at SP is most likely due to its greatly shorten chemical lifetime in the near vicinity of the plateau. It is proposed that this is due to the influence of NO on the distribution of OH in the lower free troposphere over a region that extends well beyond the plateau itself. Details related to each of the above findings plus others can be found in the 11 accompanying Special Issue papers.

Original languageEnglish (US)
Pages (from-to)5363-5373
Number of pages11
JournalAtmospheric Environment
Issue number32
StatePublished - Oct 2004

Bibliographical note

Funding Information:
The many authors of this paper would like to thank NOAA's CMDL personnel for their ready support of all our ISCAT efforts at the ARO facility at South Pole, with special thanks going to Pauline Roberts. The author D.D. Davis would also like to express his appreciation to the National Science Foundation's Office of Polar Programs (grant # OPP-9725465) and the Division of Atmospheric Chemistry for their partial support of this research. Finally, D.D. Davis would like to acknowledge the efforts of Andrea Thompson in helping with generating the tables in this paper.


  • Antarctica
  • Overview
  • Photochemistry
  • Snow emissions
  • South Pole


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