气象科技进展
氣象科技進展
기상과기진전
Advances in Meteorological Science and Technology
2013年
4期
13-17
,共5页
游然%谷松岩%郭阳%吴学宝%杨虎%陈文新
遊然%穀鬆巖%郭暘%吳學寶%楊虎%陳文新
유연%곡송암%곽양%오학보%양호%진문신
定标%风云三号(FY-3)%微波温度计(MWTS)
定標%風雲三號(FY-3)%微波溫度計(MWTS)
정표%풍운삼호(FY-3)%미파온도계(MWTS)
Calibration%FengYun-3 (FY-3)%Microwave Temperature Sounder (MWTS)
中国风云三号(FY-3)A星于2008年5月27日成功发射,其上装载的微波温度计(Microwave Temperature Sounder,MWTS)有4个通道,频率分别为50.3,53.596,54.94和57.29GHz,可提供地面至平流层下部的大气温度廓线信息。介绍了MWTS的仪器特征和定标方法,对FY-3A发射后MWTS的仪器性能相关参数的长序列特征进行了监测分析,这些参数主要包括灵敏度、冷空和内部暖黑体的计数值、仪器温度和通道增益。通过再分析资料和微波辐射传输模拟,比较了FY-3A卫星MWTS与NOAA-18卫星先进微波温度探测器(Advanced Microwave Sounder Unit-A, AMSU-A)的观测和模拟的亮温偏差。结果表明,MWTS所有通道的灵敏度值优于其指标;通道1和3的亮温偏差与AMSU-A接近;通道2和4的偏差比AMSU-A要大一些。
中國風雲三號(FY-3)A星于2008年5月27日成功髮射,其上裝載的微波溫度計(Microwave Temperature Sounder,MWTS)有4箇通道,頻率分彆為50.3,53.596,54.94和57.29GHz,可提供地麵至平流層下部的大氣溫度廓線信息。介紹瞭MWTS的儀器特徵和定標方法,對FY-3A髮射後MWTS的儀器性能相關參數的長序列特徵進行瞭鑑測分析,這些參數主要包括靈敏度、冷空和內部暖黑體的計數值、儀器溫度和通道增益。通過再分析資料和微波輻射傳輸模擬,比較瞭FY-3A衛星MWTS與NOAA-18衛星先進微波溫度探測器(Advanced Microwave Sounder Unit-A, AMSU-A)的觀測和模擬的亮溫偏差。結果錶明,MWTS所有通道的靈敏度值優于其指標;通道1和3的亮溫偏差與AMSU-A接近;通道2和4的偏差比AMSU-A要大一些。
중국풍운삼호(FY-3)A성우2008년5월27일성공발사,기상장재적미파온도계(Microwave Temperature Sounder,MWTS)유4개통도,빈솔분별위50.3,53.596,54.94화57.29GHz,가제공지면지평류층하부적대기온도곽선신식。개소료MWTS적의기특정화정표방법,대FY-3A발사후MWTS적의기성능상관삼수적장서렬특정진행료감측분석,저사삼수주요포괄령민도、랭공화내부난흑체적계수치、의기온도화통도증익。통과재분석자료화미파복사전수모의,비교료FY-3A위성MWTS여NOAA-18위성선진미파온도탐측기(Advanced Microwave Sounder Unit-A, AMSU-A)적관측화모의적량온편차。결과표명,MWTS소유통도적령민도치우우기지표;통도1화3적량온편차여AMSU-A접근;통도2화4적편차비AMSU-A요대일사。
The Chinese FengYun-3 (FY-3)A satellite was successfully launched on May 27, 2008, with a Microwave Temperature Sounder (MWTS) onboard. MWTS has four channels with frequencies of 50.3, 53.596, 54.94, and 57.29 GHz, respectively. The MWTS measurements are primarily used for profiling atmospheric temperatures from surface to lower stratosphere. MWTS is a cross-track scanning instrument, and its Earth-view measurements are calibrated through the warm target and cold space measurements during every scan cycle. In this paper, the FY-3A MWTS and its channel characteristics are first introduced. The calibration process and the postlaunch instrument performance are then presented, including the long-term trends of noise equivalent differential temperature (NEDT), calibration counts from cold space and warm targets, instrument telemetry, and channel gains. The observed and simulated brightness temperature (BT) differences of MWTS and Advanced Microwave Sounding Unit-A (AMSU-A) are compared. It is shown that the MWTS NEDT values at all channels are much better than its speciifcation. The BT biases of MWTS channels 1 and 3 with respect to the simulations are similar in magnitude to those from National Oceanic and Atmospheric Administration-18 AMSU-A. The MWTS biases at channels 2 and 4 are larger than AMSU-A.