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Calibration::Parallactic Class Reference Parallactic angle transformation of receiver feed. More...
Inheritance diagram for Calibration::Parallactic:
Detailed DescriptionParallactic angle transformation of receiver feed. The parallactic angle is also known as the Vertical Angle (VA). According to http://www.ucolick.org/~sla/deimos/swpdr/va.html "Note that in many applications this angle is mis-named the 'Parallactic Angle'. Lately this has been promoted by terminology found in the extremely useful SLALIB software by Pat Wallace, but the misnomer can be traced back at least as far as Spherical Astronomy by Smart. The correct usage of Parallactic Angle is in the context of the Equatorial and Ecliptic coordinate systems. In that context it describes the orientation of the ellipse that stellar coordinates traverse due to annual parallax. The term 'Parallactic Angle' should not be applied in the context of the Horizon system." Nevertheless, the term 'Parallactic' is used to name this class. The following description also comes from the same web-site: "The declination of an object is delta, with north being positive. The latitude of an observer is phi, with north being positive. The Hour Angle of an object is HA; zero on the meridian, negative to the east, and positive to the west. In the equatorial (RA,Dec) coordinate system the position angle of a directed vector on the sky is measured from equatorial North toward equatorial East; this is EquPA. In the Horizon (Alt-Az) coordinate system the position angle of a directed vector on the sky is measured from Up toward an upright observer's Left; this is HorPA. [...] The Vertical Angle (VA) is defined as the PA of the local vertical as expressed in the equatorial system: VA = EquPA - HorPA" This class represents the transformation from EquPA to HorPA as a rotation about the Stokes V axis by -VA. The documentation for this class was generated from the following files:
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