首页|星载微波辐射计欧洲大陆无线电频率干扰分析

星载微波辐射计欧洲大陆无线电频率干扰分析

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基于2011年6月1日至16日先进微波扫描辐射计(AMSR-E)的观测资料,采用改进的主成分分析算法,对欧洲陆地区域的无线电频率干扰(RFI)进行识别和分析.研究发现影响英国和意大利的X波段RFI源主要是稳定的、持续的地面主动源,而影响欧洲其他国家的RFI则主要是反射的静止电视卫星信号对星载微波被动传感器观测的干扰.源于静止电视卫星的RFI出现位置和强度随时间周期性变化,在欧洲陆地多出现在星载微波辐射计升轨观测上,降轨观测则几乎不受其干扰.RFI出现位置和强度与星载微波辐射计扫描方位角和观测视场相对静止电视卫星的方位有关,只有当星载微波辐射计视场扫描方位角大小与该视场相当于静止卫星发射方位角大小接近时该视场易受RFI影响.
Source Analysis of Radio-Frequency Interference over Europe Land from Advanced Microwave Scanning Radiometer-E
The radio-frequency interference (RFI) over Europe land is identified and analyzed based on advanced microwave scanning radiometer-E (AMSR-E) observations from June 1 to 16,2011 using modified principal component analysis algorithm.The X band AMSR-E measurements of England and Italy are mostly interfered by the stable,persistent active surface microwave transmitters.While the RFI source of other European countries is the interference of the reflected geostationary TV satellite downlink signals to the measurements of spaceborne microwave radiometer.The RFI location and intensity derived from the geostationary TV or communication satellite changes with time within observation period.The observations of spaceborne microwave radiometer of desending portions of orbits are usully interfered over Europe land,while ascending portions of orbits are hardly interfered.The RFI location and intensity from the reflection of downlink radiation are highly dependent upon the relative geometry between the geostationary satellite and the measuring passive sensor.Only these field of views which the scanning azimuth of spaceborne instrument is close to the relative azimuth to the geostationary satellite are easily effected by RFI.

detectorsadvanced microwave scanning radiometer-Eradio-frequency interferencygeostationary TV satellite

官莉、张思勃

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南京信息工程大学气象灾害预报预警与评估协同创新中心,中国气象局气溶胶-云-降水重点开放实验室,江苏南京210044

探测器 先进微波扫描辐射计 无线电频率干扰 静止电视卫星

国家自然科学基金江苏省高校自然科学研究重大项目江苏省普通高校研究生科研创新计划项目

4117503413KJA170003CXLX13_489

2014

光学学报
中国光学学会 中国科学院上海光学精密机械研究所

光学学报

CSTPCDCSCD北大核心EI
影响因子:1.931
ISSN:0253-2239
年,卷(期):2014.34(7)
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