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Pulsar::CalibratorStokes Class Reference Stores the Stokes parameters of the reference source. More...
Inheritance diagram for Pulsar::CalibratorStokes:
Detailed DescriptionStores the Stokes parameters of the reference source. This Archive::Extension class provides a simple container for storing the Stokes parameters of the artificial (reference) calibrator source. Member Function Documentation◆ get_coupling_point()
The point where the reference source signal is coupled. Get the name of the point where the reference source signal is coupled. References coupling_point. Referenced by Pulsar::FITSArchive::unload(). ◆ set_coupling_point()
Set the point where the reference source signal is coupled. Set the name of the point where the reference source signal is coupled. References coupling_point. Member Data Documentation◆ coupling_point
The point where the reference source signal is coupled. On some systems, the reference source (e.g. noise diode) signal is coupled to the astronomy signal after the OMT. Also, when modeling the instrumental response using METM, variable ionospheric Faraday rotation causes variable apparent rotation about the line of sight, which in turn affects the best-fit Stokes parameters of the reference source. Therefore, when using METM, it is best to model the reference source as though coupled after the frontend. Referenced by CalibratorStokes(), get_coupling_point(), operator=(), and set_coupling_point(). ◆ stokes
The Stokes parameters for each frequency channel. Stokes I is used to represent data validity Referenced by frequency_append(), get_nchan(), get_stokes(), get_valid(), operator=(), range_check(), remove_chan(), set_nchan(), set_stokes(), and set_valid(). The documentation for this class was generated from the following files:
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