Session 5.4 How well are recent climate variability signals resolved by satellite radiative flux estimates? (Invited Presentation)

Wednesday, 22 September 2004: 5:00 PM
F. R. Robertson, NASA/MSFC, Huntsville, AL; and H. I. Lu

Presentation PDF (589.8 kB)

One notable aspect of Earth’s climate is that although the planet appears to be very close to radiative balance at top-of-atmosphere (TOA), the atmosphere itself and underlying surface are not. Profound exchanges of energy between the atmosphere and oceans, land and cryosphere occur over a range of time scales. Recent evidence from broadband satellite measurements suggests that even these TOA fluxes contain some detectable variations. Our ability to measure and reconstruct radiative fluxes at the surface and at the top of atmosphere is improving rapidly. Understanding the character of radiative flux estimates and relating them to variations in other energy fluxes and climate state variables is key to improving our understanding of climate.

In this work we will evaluate two recently released estimates of radiative fluxes, focusing primarily on surface estimates. The International Satellite Cloud Climatology Project “FD” radiative flux profiles are available from mid-1983 to near present and have been constructed by driving the radiative transfer physics from the Goddard Institute for Space Studies (GISS) global model with ISCCP clouds and TOVS (TIROS Operational Vertical Sounder)thermodynamic profiles. Full and clear sky SW and LW fluxes are produced. A similar product from the NASA/GEWEX Surface Radiation Budget Project using different radiative flux codes and thermodynamics from the NASA/Goddard Earth Observing System (GEOS-1) assimilation model makes a similar calculation of surface fluxes. However this data set currently extends only through 1995.

Significant differences in both interannual variability as well as trends are found between the two data sets. These differences are traced to TOVS thermodynamic soundings used to drive the ISCCP-FD calculations. Revised estimates of clear-sky fluxes are made using statistical algorithms and water vapor from the (SSM/I) Special Sensor Microwave Imager. These calculations show strong near-surface water vapor feedback over the tropical oceans is association with SST changes. These interannual and decadal variations in fluxes are interpreted in light of recent evidence of systematic TOA flux changes over the tropics during the 1990s.

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