Coordinate Systems
The topics below discuss how Mira works with the coordinate systems of images and plots.
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 Describes the FITS World Coordinate System.  | 
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 Describes how coordinate systems are used for measuring distances, angles, centroid positions, and other quantities in images.  | 
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 Describes how pixels are referenced and counted in image coordinates.  | 
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 Describes how fractional pixels are counted in image coordinates.  | 
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 Describes how angles are measured for different coordinate systems.  | 
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 Describes how coordinate systems are used in displaying 1-D data.  | 
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 Describes how 1-D plots implement the image coordinate system.  | 
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 Describes how rows are counted in different image formats.  | 
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 Describes how FITS format images are oriented for display.  | 
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 Describes real-time readout of the image pointer (crosshair).  | 
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 Describes how to adjust and position the image cursor.  | 
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 Describes header keywords used to describe world coordinate systems.  | 
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 Configures the X world coordinate display when the X coordinate is calibrated in linear units.  | 
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 Configures the Y world coordinate display when the Y coordinate is calibrated in linear units.  | 
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 Configures the display of pixel (Z) values.  | 
The topics below discuss tools used for calibrating and working with world coordinate systems
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 Creates a "plate solution" for an image using the coordinates of at least 3 marked stars.  | 
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 Assigns an arcsecond scale to an image.  | 
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 Assigns a simple equatorial coordinate system of (right ascension, declination) to an image.  | 
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 Sets linear coordinate scales that differ in each axis.  | 
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 Sets the name for linear coordinate units in each axis.  | 
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 Deletes any type of World Coordinate System scale from the image, reverting it to the (column,row) system.  | 
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 Lists the values of world coordinate system keywords in the image header.  | 
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 Moves the image cursor to a target position, or loads the current position in either pixel or world coordinates.  |