摘要
针对8 mm波段综合孔径辐射计射频前端电尺寸较大、采用常规Y形阵列布局系统成像视场范围小的缺点,首先提出了一种星形天线阵列布局,它使可视度函数采样点之间的间隔变为天线单元间隔的一半,从而使系统的成像视场扩大到原来的两倍;然后,针对星形阵列可视度函数采样点缺失的问题,研究了背景对消与凸集投影相结合的图像反演算法,并进行了成像仿真.仿真结果验证了该反演算法的有效性.
The field of view (FOV) of the 8 mm band synthetic aperture radiometer with regular Y-shaped array is small due to the relative large electronic scale of the RF front. To overcome this disadvantage, a kind of star-shaped array is presented. In the star-shaped array, the visible distance is only half of that of the antennas, so it doubles the imaging FOV. To deal with the missing visibilities of the star-shaped array, an image restoration method based on back-dropping and projecting onto convex set (POCS) is presented. Imaging simulations were carried out. The simulations validate the effectivity of the presented method.
出处
《红外与毫米波学报》
SCIE
EI
CAS
CSCD
北大核心
2013年第1期50-55,共6页
Journal of Infrared and Millimeter Waves
基金
国家自然科学基金(61001136)~~
关键词
综合孔径
辐射计
图像反演
synthetic aperture
radiometer
image restoration