Earth's Infrared Background
Ofer Shamir, Edwin P. Gerber
Comments 15 pages, 8 figures
详情
Much of the Outgoing Longwave Radiation (OLR) emitted to space is best described as random variability, or the ``Earth's Infrared Background''. A rigorous characterization of this background provides an objective null hypothesis and enables the isolation of atmospheric phenomena -- such as waves, storms, and other coherent structures -- within OLR observations. To this end, we identify the background as isotropic fluctuations implied by the fluctuation-dissipation theorem in response to internal atmospheric variability on small spatiotemporal scales. We use a stochastically forced energy balance climate model, which has a broad sense red spectrum consistent with observations, a first-order process in time, and a second-order process in space. By fitting the model to OLR data from satellite observations, we find that the background fluctuations have an upper bound of about 400~km and 2.5~days on their spatiotemporal (de)correlations, between meso-scale and synoptic-scale weather.