Use of a GCM to explore sampling issues in connection with satellite remote sensing of the Earth radiation budget

Citation
Ld. Fowler et al., Use of a GCM to explore sampling issues in connection with satellite remote sensing of the Earth radiation budget, J GEO RES-A, 105(D16), 2000, pp. 20757-20772
Citations number
40
Categorie Soggetti
Earth Sciences
Volume
105
Issue
D16
Year of publication
2000
Pages
20757 - 20772
Database
ISI
SICI code
Abstract
Collocated in time and space, top-of-the-atmosphere measurements of the Ear th radiation budget (ERB) and cloudiness from passive scanning radiometers, and lidar- and radar-in-space measurements of multilayered cloud systems, are the required combination to improve our understanding of the role of cl ouds and radiation in climate. Experiments to fly multiple satellites "in f ormation" to measure simultaneously the radiative and optical properties of overlapping cloud systems are being designed. Because satellites carrying ERB experiments and satellites carrying lidars- or radars-in space have dif ferent orbital characteristics, the number of simultaneous measurements of radiation and clouds is reduced relative to the number of measurements made by each satellite independently. Monthly averaged coincident observations of radiation and cloudiness are biased when compared against more frequentl y sampled observations due, in particular, to the undersampling of their di urnal cycle. Using the Colorado State University General Circulation Model (CSU GCM), the goal of this study is to measure the impact of using simulta neous observations from the Earth Observing System (EOS) platform and compa nion satellites flying lidars or radars on monthly averaged diagnostics of longwave radiation, cloudiness, and its cloud optical properties. To do so, the hourly varying geographical distributions of coincident locations betw een the afternoon EOS (EOS-PM) orbit and the orbit of the ICESAT satellite set to fly at the altitude of 600 km, and between the EOS PM orbit and the orbits of the PICASSO satellite proposed to fly at the altitudes of 485 km (PICA485) or 705 km (PICA705), are simulated in the CSU GCM for a 60-month time period starting at the idealistic July 1, 2001, launch date. Monthly a veraged diagnostics of the top-of-the-atmosphere, atmospheric, and surface longwave radiation budgets and clouds accumulated over grid boxes correspon ding to satellite overpasses are compared against monthly averaged diagnost ics obtained from hourly samplings over the entire globe. Results show that differences between irregularly (satellite) and regularly (true) sampled d iagnostics of the longwave net radiative budgets are the greatest at the su rface and the smallest in the atmosphere and at the top-of-the-atmosphere, under both cloud-free and cloudy conditions. In contrast, differences betwe en the satellite and the true diagnostics of the longwave cloud radiative f orcings are the largest in the atmosphere and at the top-of-the atmosphere, and the smallest at the surface. A poorer diurnal sampling of the surface temperature in the satellite simulations relative to the true simulation co ntributes a major part to sampling biases in the longwave net radiative bud gets, while a poorer diurnal sampling of cloudiness and its optical propert ies directly affects diagnostics of the longwave cloud radiative forcings. A factor of 8 difference in the number of satellite overpasses between PICA 705 and PICA485 and ICESAT leads to a systematic factor of 3 difference in the spatial standard deviations of all radiative and cloudiness diagnostics .