| Atmospheric Correction Of Imaging Spectrometer On (2007) | |||||||||||||
Abstract | |||||||||||||
| the laboratory spectrum. Major sources of arc shown to arise from atmospheric gaseous absorption and solar file used in the transfer code as well as uncertainties in instrument calibration coefficients, particularly visible part of spectrum and around 1200 nm. Generalization to an entire scene implies on a by-pixel basis of ground elevation, viewing geometry, water vapor content and estimated ground Systematic departure from mode] assumptions main] y translate in the reflectance into residual absorption or spikes corresponding or for atmospheric gases. 1. Wc report here preliminary results on our assessment of the accuracy of an for atmospheric correction of high spectral resolution imaging data. is based on a model of radiance each wavelength the sensor that approximately written: Subscript AV refers is path and "1', the diffuse direct transmitted radiance atmosphere and arc using radiative codes 7 | |||||||||||||
Publication details | |||||||||||||
| |||||||||||||