INTERCALIBRATING THE GPM CONSTELLATION USING THE GPM MICROWAVE IMAGER (GMI)

被引：0

作者：

Wilheit, Thomas ^{[1
]}

Berg, Wesley ^{[2
]}

Ebrahimi, Hamideh ^{[3
]}

Kroodsma, Rachael ^{[4
]}

McKague, Darren ^{[5
]}

Payne, Vivienne ^{[6
]}

Wang, James

机构：

[1] Texas A&M Univ, College Stn, TX 77843 USA

[2] Colorado State Univ, Ft Collins, CO 80523 USA

[3] Univ Cent Florida, Orlando, FL 32816 USA

[4] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA

[5] Univ Michigan, Ann Arbor, MI 48109 USA

[6] CALTECH, Jet Prop Lab, Pasadena, CA 91125 USA

来源：

2015 IEEE INTERNATIONAL GEOSCIENCE AND REMOTE SENSING SYMPOSIUM (IGARSS) | 2015年

关键词：

Calibration; Microwave radiometry; Satellites; WATER-VAPOR PROFILES; CALIBRATION; RADIOMETERS; RETRIEVAL;

D O I：

暂无

中图分类号：

TM [电工技术]; TN [电子技术、通信技术];

学科分类号：

0808 ; 0809 ;

摘要：

A constellation of disparate radiometers is inherent to the Global Precipitation Measurement (GPM) mission concept. The task of the Intersatellite Calibration Working group is to generate adjustments to make the measurements of all these radiometers physically consistent. A key role of the GPM Microwave Imager (GMI) on the GPM Core satellite is to serve as a transfer standard among the constellation radiometers. The TRMM Microwave Imager (TMI) has served this role during the development phase and for interim corrections early in the GPM mission. The stability of GMI appears to be very good and a physically based calibration has been generated that appears to be accurate at the 1K level or better.

引用

页码：5162 / 5165

页数：4

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