Aquarius Scatterometer Calibration

被引:5
|
作者
Fore, Alexander G. [1 ]
Neumann, Gregory [1 ]
Freedman, Adam P. [1 ]
Chaubell, Mario Julian [1 ]
Tang, Wenqing [1 ]
Hayashi, Akiko K. [1 ]
Yueh, Simon H. [1 ]
机构
[1] CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91109 USA
关键词
Aquarius; backscatter; L-band; ocean winds; radar; remote sensing; scatterometery; WIND-SPEED; SALINITY;
D O I
10.1109/JSTARS.2015.2493449
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
In this paper, we discuss the Aquarius scatterometer calibration, starting with the instrument calibration. We examine the stability of Aquarius as quantified using the loop-back power and estimated receiver gain to shown Aquarius has been extremely stable to order 0.1 dB since mission start. We show the temperatures of scatterometer components not contained in the loop-back path have been controlled precisely to 0.5 degrees C to minimize any temperature-dependent losses. Combined, these results show Aquarius produces accurate sigma(0) over the mission lifetime. In the next section, we discuss the stability as quantified using external models and again show stability to order 0.1 dB in very good agreement with instrument-only methods. Then, we discuss the methods used to absolutely calibrate Aquarius sigma(0) with respect to previous L-band radar systems. We show that Aquarius is relatively calibrated to order 0.1 dB for copolarization channels and better than 0.2 dB for cross-polarization channels. Finally, we discuss the calibration of the Aquarius wind speed product. We compare the Aquarius wind speed with radiometer wind speed products, other radar scatterometers, and numerical weather products. We show that the Aquarius wind speed product is on par with previous scatterometers in data quality.
引用
收藏
页码:5424 / 5432
页数:9
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