Detection of 2002-2003 El Ni${\tilde{n}}$o Using EOS and OSMI Data

  • Lee, S.H. (Satellite Operation & Application Center, Korea Aerospace Research Institute) ;
  • Lim, H.S. (Satellite Operation & Application Center, Korea Aerospace Research Institute) ;
  • Kim, J.G. (Satellite Operation & Application Center, Korea Aerospace Research Institute) ;
  • Jun, J.N. (Satellite Operation & Application Center, Korea Aerospace Research Institute)
  • Published : 2003.11.03

Abstract

Interannual variability in the patterns of satellitederived pigment concentrations, sea-level height anomaly, sea surface temperature anomaly, and zonal wind anomaly are observed during the 2002-2003 El Ni${\tilde{n}}$o. The largest spatial extent of the phytoplankton bloom was recovery from El Ni${\tilde{n}}$o over the equatorial Pacific. The evolution towards a warm episode (El Ni${\tilde{n}}$o) started from spring of 2002 and continued during January 2003, while equatorial Sea Surface Temperature Anomaly (SSTA) remained greater than +1$^{\circ}$C in the central equatorial Pacific. The EOS (Earth Observing System) and OSMI (Ocean Scanning Multispectral Imager) data are used for detection of dramatic changes in the patterns of pigment concentration during El Ni${\tilde{n}}$o.

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