Leonard W. Abreu
Philips
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Featured researches published by Leonard W. Abreu.
Proceedings of SPIE | 1993
Gail P. Anderson; James H. Chetwynd; Jean-Marc Thériault; Prabhat K. Acharya; Alexander Berk; David C. Robertson; F. X. Kneizys; Michael L. Hoke; Leonard W. Abreu; Eric P. Shettle
MODTRAN2 (1992) is the most recent version of MODTRAN, the Moderate Resolution Atmospheric Radiance and Transmittance Model, first released by the Geophysics Directorate, Phillips Laboratory, in 1990. It encompasses all the capabilities of LOWTRAN 7, the historic 20 cm-1 resolution radiance code, but incorporates a much more sensitive molecular band model with 2 cm-1 resolution. For inversion algorithm applications, MODTRAN2 must prove to be sufficiently accurate when calculating layer- specific perturbations. First steps in establishing this capability have recently been accomplished. DREV (Defence Research Establishment Valcartier, Canada), in conjunction with the Geophysics Directorate, has taken measurements with a surface-based Bomem interferometer (approximately 1 cm-1 resolution), with full supporting sonde profiles (z, T, p, and relative humidity). This suggests that the derivative matrices, typically required for inversion algorithms, may be readily (and rapidly) calculated using MODTRAN whenever its spectral resolution is adequate.
Passive Infrared Remote Sensing of Clouds and the Atmosphere II | 1994
Gail P. Anderson; Jinxue Wang; Michael L. Hoke; F. X. Kneizys; James H. Chetwynd; Laurence S. Rothman; L. M. Kimball; Robert A. McClatchey; Eric P. Shettle; Shepard A. Clough; William O. Gallery; Leonard W. Abreu; John E. A. Selby
Beginning in the early 1970s, the then Air Force Cambridge Research Laboratory initiated a program to develop computer-based atmospheric radiative transfer algorithms. The first attempts were translations of graphical procedures described in a 1970 report on The Optical Properties of the Atmosphere, based on empirical transmission functions and effective absorption coefficients derived primarily from controlled laboratory transmittance measurements. The fact that spectrally-averaged atmospheric transmittance (T) does not obey the Beer-Lambert Law (T equals exp(-(sigma) (DOT)(eta) ), where (sigma) is a species absorption cross section, independent of (eta) , the species column amount along the path) at any but the finest spectral resolution was already well known. Band models to describe this gross behavior were developed in the 1950s and 60s. Thus began LOWTRAN, the Low Resolution Transmittance Code, first released in 1972. This limited initial effort has how progressed to a set of codes and related algorithms (including line-of-sight spectral geometry, direct and scattered radiance and irradiance, non-local thermodynamic equilibrium, etc.) that contain thousands of coding lines, hundreds of subroutines, and improved accuracy, efficiency, and, ultimately, accessibility. This review will include LOWTRAN, HITRAN (atlas of high-resolution molecular spectroscopic data), FASCODE (Fast Atmospheric Signature Code), and MODTRAN (Moderate Resolution Transmittance Code), their permutations, validations, and applications, particularly as related to passive remote sensing and energy deposition.
Optical Spectroscopic Techniques and Instrumentation for Atmospheric and Space Research II | 1996
Gail P. Anderson; F. X. Kneizys; James H. Chetwynd; Laurence S. Rothman; Michael L. Hoke; Alexander Berk; Lawrence S. Bernstein; Prabhat K. Acharya; Hilary E. Snell; Eli J. Mlawer; Shepard A. Clough; Jinxue Wang; S. Y. Lee; Henry E. Revercomb; Tatsuya Yokota; L. M. Kimball; Eric P. Shettle; Leonard W. Abreu; John E. A. Selby
Spectrally uniform treatment of the atmospheric radiative transfer (RI) problem has been approached through two different techniques - very high resolution line-by-line (LBL) algorithms and lower resolution band models (BM). Each has its advantages and specific applications. However, if commonality and validation of a specific pair of RI approaches is to be mutually maintained, then these codes must be continually reevaluated against both measurements and other models.
1982 Technical Symposium East | 1982
Vincent J. Falcone; Leonard W. Abreu; Eric P. Shettle
Radiative transfer in the earths atmosphere is modeled by a computer code called RADTRAN. RADTRAN may be used to model atmospheric transmission and emission in the frequency range of 30-300 GHz. Two versions of this computer code exist: the first is RADTRAN which incorporates six model clear atmospheres, six cloud models, six rain models and eight humidity models to model worldwide atmospheric conditions; the second is MWTRAN which is approximately one-sixth of the physical size of RADTRAN. Both RADTRAN and MWTRAN allow the researcher to read in any model data in any format.
1980 Huntsville Technical Symposium | 1981
Vincent J. Falcone; Leonard W. Abreu
Atmospheric models of fog, clouds and rain are described. These models are typical for mid-latitude temperate regions of the globe. A computer code for incorporating the models into a new efficient computer algorithm of the AFGL HITRAN series named FASCOD1 has been completed. The computer models presented allow calculation of atmospheric transmission or attenuation for millimeter and submillimeter waves (1-34 cm-1 or 1-1000 GHz). Four (4) fog models, eight (8) cloud types and rainfall rates from 1-150 mm hr available. All models consider hydrometeors as having temperatures between 0°C and 40°C and permit arbitrary input of atmospheric parameters and geometry (slant range).
Archive | 1979
Vincent J. Falcone; Leonard W. Abreu; Eric P. Shettle
Archive | 1991
Leonard W. Abreu; Francis X. Kneizys; Gail P. Anderson; James H. Chetwynd; Lex Berk; Larry S. Bernstein; David C. Robertson
Archive | 1989
Francis X. Kneizys; Eric P. Shettle; Leonard W. Abreu; James H. Chetwynd; Gail P. Anderson; William O. Gallery; John E. A. Selby; Shepard A. Clough
Archive | 1990
Gail P. Anderson; Francis X. Kneizys; Eric P. Shettle; Leonard W. Abreu; James H. Chetwynd; Robert E. Huffman; L. A. Hall
Archive | 1990
Francis X. Kneizys; Gail P. Anderson; Eric P. Shettle; Leonard W. Abreu; James H. Chetwynd; John E. A. Selby; William O. Gallery; Shepard A. Clough