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High power amplifier is a very significant component in satellite communication and it is very important to analyze its performance according to the satellite application it is used in. Noise power ratio, also known as carrier to inter-modulation noise ratio is an important parameter for analyzing the performance of high power amplifiers. All power amplifiers are nonlinear to some degree. If more than one carrier is received by a single amplifier, mixing or inter-modulation processes will take place. The inter-modulation analysis becomes complex as the number of carriers are increased in the…mehr

Produktbeschreibung
High power amplifier is a very significant component in satellite communication and it is very important to analyze its performance according to the satellite application it is used in. Noise power ratio, also known as carrier to inter-modulation noise ratio is an important parameter for analyzing the performance of high power amplifiers. All power amplifiers are nonlinear to some degree. If more than one carrier is received by a single amplifier, mixing or inter-modulation processes will take place. The inter-modulation analysis becomes complex as the number of carriers are increased in the transmitted signal. In order to analyse inter-modulation distortion products, NPR measurement technique is employed. The book highlights the significance of NPR measurement and also provides MATLAB based simulated results of noise power ratio measurement using high power amplifier models. The simulated results are compared with the actual results and the accuracy of the simulator along with the amount of systematic error is determined for every IPBO value.
Autorenporträt
Adnan Zafar received his Bachelor of Science Degree in Communication Systems Engineering from Institute of Space Technology,Pakistan and Master of Science Degree in Satellite Communications Engineering from University of Surrey,United Kingdom. He is currently working as lecturer in Electrical Engineering Department of Institute of Space Technology.