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NASA NTRS · 20100032967

Phased Array Radiometer Calibration Using a Radiated Noise Source

Abstract

Electronic beam steering capability of phased array antenna systems offer significant advantages when used in real aperture imaging radiometers. The sensitivity of such systems is limited by the ability to accurately calibrate variations in the antenna circuit characteristics. Passive antenna systems, which require mechanical rotation to scan the beam, have stable characteristics and the noise figure of the antenna can be characterized with knowledge of its physical temperature [1],[2]. Phased array antenna systems provide the ability to electronically steer the beam in any desired direction. Such antennas make use of active components (amplifiers, phase shifters) to provide electronic scanning capability while maintaining a low antenna noise figure. The gain fluctuations in the active components can be significant, resulting in substantial calibration difficulties [3]. In this paper, we introduce two novel calibration techniques that provide an end-to-end calibration of a real-aperture, phased array radiometer system. Empirical data will be shown to illustrate the performance of both methods.

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BibTeXRIS

Srinivasan, Karthik, Limaye, Ashutoch S., Laymon, Charles A., Meyer, Paul J.. 2010-07-25. Phased Array Radiometer Calibration Using a Radiated Noise Source. https://ntrs.nasa.gov/citations/20100032967

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