Difference between revisions of "Basic Interferometry"

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A two-element interferometer consists of two telescopes seperated by a distance $\mathbf{b}$, called the baseline.  Both antennas receive electromagnetic radiation from an astronomical source in the sky.   
 
A two-element interferometer consists of two telescopes seperated by a distance $\mathbf{b}$, called the baseline.  Both antennas receive electromagnetic radiation from an astronomical source in the sky.   
Because astronomical sources are far away, the radiation received is in the form of plane waves.   
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Because astronomical sources are far away, the radiation received by the antennas is in the form of plane waves. As the plane waves reach the antennas,  one will actually receive the signal first and the second will not receive the signal until a certain amount of time has passed.  The 
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%\subsection*{Why Interfeormetry?}
 
%\subsection*{Why Interfeormetry?}
  

Revision as of 11:38, 12 September 2011

Basic Interferometry

Interferometry is the practice of using a two-or-more-element radio telescope array to observe astronomical sources. The array itself, along with the electronics used to synthesise the signals detected by the telescopes, are what we call the interferometer.

A two-element interferometer consists of two telescopes seperated by a distance , called the baseline. Both antennas receive electromagnetic radiation from an astronomical source in the sky. Because astronomical sources are far away, the radiation received by the antennas is in the form of plane waves. As the plane waves reach the antennas, one will actually receive the signal first and the second will not receive the signal until a certain amount of time has passed. The