Sunday, December 30, 2007

Software Correlator - II

The angular resolution of radio telescopes can be improved by using the principles of interferometry. Interferometry depends upon detecting the combination of voltage signals assumed to be originating from the same source. In a simple two-element radio interferometer, the signals from a point source alternately arrive in phase and out of phase as the Earth rotates and causes a change in the difference in path from the radio source to the two elements of the interferometer. This produces interference fringes in a manner similar to that in Young's double-slit interference experiment, shown below.





The figure below shows how two waves from the same point source reach the two antennas on ground with a certain geometric path difference. If we multiple the two voltages generated at the antennas due to the waves reaching their respective locations, an interference pattern is observed (see third figure further down). Note how the appearance is exactly identical to the interference pattern generated by a two-slit interferometer using two slits as point sources, shown above.





The 'geometric' path difference due to spatial orientation of the source is similar to the path difference in 2-slit interference experiment. We probe phenomenon of 'temporal coherence' in 2-slit Young's experiment, that is we study the stability of phase difference between two sources (slits) over time. If the phase difference betwee two slits varied randomly, fringes will not have any absolute dark fringe ('zero' of intensity).





On the other hand, in 2-antenna interference,
the phase difference arises due to different locations of the 2 antennas as seen by the source. If the source was not a point source on the sky, fringes will not be perfect (no absolute zero of intensity). Thus, we study 'spatial coherence' of waves, that is if our source has a finite size.

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