TES Science Investigator-led Processing System

被引：4

作者：

Chu, E

Tremblay, D

Croft, K

Griffin, A

机构：

[1] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA

[2] Raytheon ITSS, Pasadena, CA 91101 USA

来源：

IEEE TRANSACTIONS ON GEOSCIENCE AND REMOTE SENSING | 2006年 / 44卷 / 05期

关键词：

atmospheric measurements; calibration; computer; architecture; computer facilities; data processing; Fourier spectroscopy; Fourier transform; multiprocessing; optical interferometry; parallel processing; processor scheduling; spectroscopy; terrestrial atmosphere;

D O I：

10.1109/TGRS.2005.863713

中图分类号：

P3 [地球物理学]; P59 [地球化学];

学科分类号：

0708 ; 070902 ;

摘要：

The Tropospheric Emission Spectrometer (TES) is one of four instruments onboard the Earth Observing System Aura satellite. The TES Science Investigator-led Processing System (SIPS) Facility performs production processing of all TES science data. When the TES project was proposed in 1988, its science algorithms were still evolving, but it was already understood to be at least two orders of magnitude more complex than its NASA predecessor, the Atmospheric Trace Molecule Spectroscopy (ATMOS) instrument. In addition, the expected data volume of the TES instrument would be more than 1000 times greater than that of ATMOS. Development of the TES S I PS faced a number of technical challenges. It also would have been impractical and prohibitively costly to develop the TES SIPS facility without carefully deploying the computing technologies that have recently become available. This paper describes how the challenges were met in the development of the facility by making use of evolving hardware technology and software refinement. The process revealed that the architecture of the hardware implemented was highly dependent upon the processing algorithm, and a stable algorithm was needed early in the hardware development process for performance analysis and benchmarking.

引用

页码：1352 / 1358

页数：7

共 10 条

[1] Tropospheric emission spectrometer for the Earth Observing System's Aura Satellite [J].

Beer, R ;

Glavich, TA ;

Rider, DM .

APPLIED OPTICS, 2001, 40 (15) :2356-2367

[2]

BEER R, 1999, TES LEVEL 2 ALGORITH

[3]

BOWMAN KW, 2004, D16479 JPL

[4]

FARMER CB, 1989, NASA REF PUB, V1224

[5]

Marks Robert J., 1991, Introduction to Shannon Sampling and Interpolation Theory

[6] TES ground data system software [J].

Paradise, S ;

Akopyan, S ;

De Baca, RC ;

Croft, K ;

Fry, K ;

Gluck, S ;

Ho, D ;

Koffend, B ;

Lampel, M ;

McDuffie, J ;

Monarrez, R ;

Nair, H ;

Poosti, S ;

Shepard, D ;

Strickland, I ;

Tremblay, D ;

Yun, H ;

Zong, J .

IEEE TRANSACTIONS ON GEOSCIENCE AND REMOTE SENSING, 2006, 44 (05) :1343-1351

[7] RADIOMETRIC CALIBRATION OF IR FOURIER-TRANSFORM SPECTROMETERS - SOLUTION TO A PROBLEM WITH THE HIGH-RESOLUTION INTERFEROMETER SOUNDER [J].

REVERCOMB, HE ;

BUIJS, H ;

HOWELL, HB ;

LAPORTE, DD ;

SMITH, WL ;

SROMOVSKY, LA .

APPLIED OPTICS, 1988, 27 (15) :3210-3218

[8] The HITRAN molecular spectroscopic database: edition of 2000 including updates through 2001 [J].

Rothman, LS ;

Barbe, A ;

Benner, DC ;

Brown, LR ;

Camy-Peyret, C ;

Carleer, MR ;

Chance, K ;

Clerbaux, C ;

Dana, V ;

Devi, VM ;

Fayt, A ;

Flaud, JM ;

Gamache, RR ;

Goldman, A ;

Jacquemart, D ;

Jucks, KW ;

Lafferty, WJ ;

Mandin, JY ;

Massie, ST ;

Nemtchinov, V ;

Newnham, DA ;

Perrin, A ;

Rinsland, CP ;

Schroeder, J ;

Smith, KM ;

Smith, MAH ;

Tang, K ;

Toth, RA ;

Vander Auwera, J ;

Varanasi, P ;

Yoshino, K .

JOURNAL OF QUANTITATIVE SPECTROSCOPY & RADIATIVE TRANSFER, 2003, 82 (1-4) :5-44

[9] TES level 1 algorithms: Interferogram processing, geolocation, radiometric, and spectral calibration [J].

Worden, H ;

Beer, R ;

Bowman, KW ;

Fisher, B ;

Luo, M ;

Rider, D ;

Sarkissian, E ;

Tremblay, D ;

Zong, J .

IEEE TRANSACTIONS ON GEOSCIENCE AND REMOTE SENSING, 2006, 44 (05) :1288-1296

[10]

WORDEN HM, 1999, D16479 JPL

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