Authors: Sai Venkatesh Balasubramanian
Radio astronomy plays a crucial role in revealing vital information about the early universe and celestial structures. A novel nonlinear analysis technique using the polar and phase plane plots for analyzing radio astronomical data is proposed, and the analysis for a pulsar B1933 is performed. It is observed that the analysis reveals information regarding the angle of emissions/ beaming of 30 degrees, and this forms the novelty of the present work.
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[v1] 2015-10-27 21:18:58
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