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SUNDAZEL(1)			  User Commands 		     SUNDAZEL(1)

NAME
     sundazel - Compute the time of Solar passage

SYNOPSIS
     sundazel [<option>] [<yyyymmdd>]

DESCRIPTION
     sundazel computes the local time of the Sun's passage through the specified
     apparent longitude or latitude in a user-defined coordinate system, for the
     specified location on the specified date (default today).

     The  Sun's  apparent  hour angle, azimuth, elevation, and the longitude and
     latitude in user coordinates are also printed, in degrees.   Refraction  is
     accounted for.

     sundazel may also be used to compute the time of sunrise and set, the Sun's
     right ascension and declination, and the Equation of Time.

OPTIONS
     -p <option>

	    The Solar passage required and, if relevant, the coordinate value in
	    degrees:

     sunrise
	    Sunrise.

     sunset
	    Sunset.

     lng=<lng>
	    Longitude of the Sun in the user-defined coordinate system.

     lat=<lat>
	    Latitude of the Sun in the user-defined coordinate system.

     -l <lng>,<lat>

	    Longitude and latitude of the observer.

     -t <tz>

	    The observer's time zone, positive east of Greenwich (hr).

     -u <az>,<el>,<zlng>

	    Azimuth  and  elevation  of  the pole of the user-defined coordinate
	    system, and the longitude of the zenith (deg).  See below.

     -n     Set the user-defined coordinate system as one with pole due north on
	    the horizon, with zero of longitude at the zenith.

     -w     Set the user-defined coordinate system as one with pole due west  on
	    the horizon, with zero of longitude at the zenith.

     -v     Also  print  the  Sun's  right ascension, declination (deg), and the
	    Equation of Time (min).

     The user-defined coordinate system is a right-handed  spherical  coordinate
     system  with  its	pole  at  the  specified azimuth and elevation, and with
     zenith having the specified  longitude.   If  omitted,  the  default  is  a
     right-handed  system  with  its  pole  at the zenith and prime meridian due
     north, i.e. similar to azimuth and  elevation  except  that  longitude  in-
     creases  in  the  reverse	sense  to  azimuth, i.e. from north through west
     rather than north through east.

     Setting a range of azimuth or elevation often provides a poor criterion for
     timing the passage of the Sun, for example in determining	when  it  shines
     directly through a skylight, or when an awning casts a shadow on a particu-
     lar  point  on the ground.  In such cases the projection of the skylight or
     awning from the ground onto the sky should be considered.	Some other coor-
     dinate system may provide a better fit to the region of the sky thereby de-
     fined.  For example, the passage of the Sun across a skylight  oriented  at
     azimuth  alpha  might  be	handled via a coordinate system with pole on the
     horizon at that azimuth and considering the Sun's passage through	a  range
     of  longitude  in this system.  Perhaps better might be to use a coordinate
     system with pole at alpha-90 and considering a range of latitude.

     Sunrise and sunset correspond to first/last contact of the  Sun's	limb  on
     the  horizon, corresponding to apparent elevation -0.27 deg (true elevation
     -0.79 deg).  If no options are specified, the default is to  calculate  the
     time  of  sunset.	If more than one p option is specified, only the last is
     effective.

sundazel 8.9			    June 2026			     SUNDAZEL(1)

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