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WCSSPH2XY

WCSSPH2XY

Name


    WCSSPH2XY

Purpose


    Convert spherical coordinates to x and y (map) angular coordinates

Explanation


    Convert spherical (longitude and latitude -- sky) coordinates to x
    and y intermediate world coordinates (still nominally in degrees) in
    the projection plane of the map. This procedure is the inverse of
    WCSXY2SPH. See WCS_DEMO for example of use.
    This is a lower level procedure -- given a FITS header, the user will
    usually use ADXY which will then call WCSSPH2XY with the appropriate
    parameters.

Category


    Mapping and Auxiliary FITS Routine

Calling Sequence


      wcssph2xy, longitude, latitude, x, y, [ map_type , CTYPE = ,
              FACE =, PV1= PV2= , CRVAL = , CRXY = , LONGPOLE = ,
              LATPOLE = , PHI0 = , NORTH_OFFSET =, SOUTH_OFFSET =, BADINDEX =]

Input Parameters


    longitude - longitude of data, scalar or vector, in degrees
    latitude - latitude of data, same number of elements as longitude,
                in degrees
    map_type - optional positional parameter, numeric scalar (0-26)
              corresponding to a particular map projection. This is not a
              FITS standard, it is simply put in to allow function similar
              to that of less general map projection procedures (eg AITOFF).
              The following list gives the map projection types and their
              respective numbers.
  FITS Number Name Comments
  code code
  ---- ------ ----------------------- -----------------------------------
  DEF 0 Default = Plate Carree
  AZP 1 Zenithal perspective PV2_1 required
  TAN 2 Gnomic AZP w/ mu = 0
  SIN 3 Orthographic PV2_1,PV2_2 optional
  STG 4 Stereographic AZP w/ mu = 1
  ARC 5 Zenithal Equidistant
  ZPN 6 Zenithal polynomial PV2_0, PV2_1....PV2_20 possible
  ZEA 7 Zenithal equal area
  AIR 8 Airy PV2_1 required
  CYP 9 Cylindrical perspective PV2_1 and PV2_2 required
  CAR 10 Plate Carree
  MER 11 Mercator
  CEA 12 Cylindrical equal area PV2_1 required
  COP 13 Conical perspective PV2_1 and PV2_2 required
  COD 14 Conical equidistant PV2_1 and PV2_2 required
  COE 15 Conical equal area PV2_1 and PV2_2 required
  COO 16 Conical orthomorphic PV2_1 and PV2_2 required
  BON 17 Bonne's equal area PV2_1 required
  PCO 18 Polyconic
  SFL 19 Sanson-Flamsteed (GLS is allowed as a synonym for SFL)
  PAR 20 Parabolic
  AIT 21 Hammer-Aitoff
  MOL 22 Mollweide
  CSC 23 Cobe Quadrilateralized convergence of inverse is poor
                Spherical Cube
  QSC 24 Quadrilateralized
                Spherical Cube
  TSC 25 Tangential Spherical Cube
  SZP 26 Slant Zenithal Projection PV2_1,PV2_2, PV2_3 optional
  HPX 27 HealPix
  HCT 28 HealCart (Cartesian approximation of Healpix)
  XPH 29 HEALPix butterfly projection

Optional Input Keyword Parameters



    CTYPE - One, two, or three element vector containing 8 character
              strings corresponding to the CTYPE1, CTYPE2, and CTYPE3
              FITS keywords:
              CTYPE[0] - first four characters specify standard system
              ('RA--','GLON' or 'ELON' for right ascension, Galactic
              longitude or ecliptic longitude respectively), second four
              letters specify the type of map projection (eg '-AIT' for
              Aitoff projection)
              CTYPE[1] - first four characters specify standard system
              ('DEC-','GLAT' or 'ELAT' for declination, galactic latitude
              or ecliptic latitude respectively; these must match
              the appropriate system of ctype1), second four letters of
              ctype2 must match second four letters of ctype1.
              CTYPE[2] - if present must be the 8 character string,'CUBEFACE',
                only used for spherical cube projections to identify an axis
              as containing the face on which each x and y pair of
              coordinates lie.
    PV2 - Vector of projection parameter associated with latitude axis
            PV2 will have up to 21 elements for the ZPN projection, up to 3
            for the SIN projection and no more than 2 for any other
            projection. The first element corresponds to PV2_1, the
            second to PV2_2, etc.
    CRXY - 2 element vector giving the x and y coordinates of the
              reference point. if this is not set the offset is [0,0].
              Used to implement (x0,y0) in Sect 2.5 of Griesen & Calabretta 2002
              Do not confuse with CRPIX.
    Parameters simply passed to WCS_ROTATE:
 
    CRVAL - 2 element vector containing standard system coordinates (the
              longitude and latitude) of the reference point
    PV1 - Vector of projection parameters associated with longitude
    LONGPOLE - native longitude of standard system's North Pole
    LATPOLE - "target" native latitude of the standard system's North Pole
    Parameters intended to enhance invertability:
    NORTH_OFFSET - offset (radians) added to input points near north pole.
    SOUTH_OFFSET - offset (radians) added to input points near south pole.

Output Parameters



      x - x coordinate of data, same number of elements as longitude, in
              degrees; if CRXY is set, then x will be returned offset by
              crxy(0). NOTE: x in all map projections increases to the
              left, not the right.
      y - y coordinate of data, same number of elements as longitude, in
              degrees; if CRXY is set, y will be returned offset by crxy[1]
  OPTIONAL OUTPUT KEYWORD PARAMETERS:
      FACE - a output variable used for spherical cube projections to
              designate the face of the cube on which the x and y
              coordinates lie. Will contain the same number of elements as
              X and Y. Must contain at least 1 arbitrary element on input
              If FACE is NOT defined on input, it is assumed that the
              spherical cube projection is laid out over the whole sky
              in the "sideways T" configuration.
    BADINDEX - vector, list of transformed points too close to poles.

Notes


      The conventions followed here are described in more detail in
      "Representations of Celestial Coordinates in FITS" by Calabretta
      and Greisen (2002, A&A, 395, 1077; also see
      http://fits.gsfc.nasa.gov/fits_wcs.html). The general
      scheme outlined in that article is to first use WCS_ROTATE to convert
      coordinates in one of three standard systems (celestial, galactic,
      or ecliptic) into a "native system" of latitude and longitude. The
      latitude and longitude are then converted into x and y coordinates
      which depend on the map projection which is performed. The rotation
      from standard to native coordinates can be skipped if one so desires.
      This procedure necessitates two basic sections. The first converts
      "standard" coordinates to "native" coordinates while the second converts
      "native" coordinates to x and y coordinates. The first section is
      simply a call to WCS_ROTATE, while the second contains the guts of
      the code in which all of the map projection is done. This procedure
      can be called in a form similar to AITOFF, EQPOLE, or QDCB by calling
      wcssph2xy with a fifth parameter specifying the map projection by
      number and by not using any of the keywords related to the map
      projection type (e.g. CTYPE).

Procedure



      The first task of the procedure is to do general error-checking to
      make sure the procedure was called correctly and none of the
      parameters or keywords conflict. This is particularly important
      because the procedure can be called in two ways (either using
      FITS-type keywords or using a number corresponding to a map projection
      type). All variables are converted into double precision values and
      angular measurements are converted from degrees into radians.
      If necessary, longitude values are converted into the range -pi to pi.
      Any latitude points close to the of the poles are mapped to a specific
      latitude of from the pole so that the map transformations become
      completely invertible. The magnitude of this correction is given by
      the keywords NORTH_OFFSET and SOUTH_OFFSET and a list of affected
      points is optionally returned in the "badindex" output parameter.
      The next task of the procedure is to convert the "standard"
      coordinates to "native" coordinates by rotating the coordinate system.
      This rotation is performed by the procedure WCS_ROTATE and is governed
      by the keywords CRVAL and LONGPOLE. The final task of the WCSSPH2XY
      is to take "native" latitude and longitude coordinates and convert
      them into x and y coordinates. Any map specific error-checking is
      done at this time. All of the equations were obtained from
      "Representations of Celestial Coordinates in FITS" and cases needing
      special attention are handled appropriately (see the comments with
      individual map projections for more information on special cases).
      Note that a further transformation (using the CD matrix) is required
      to convert the (x,y) coordinates to pixel coordinates.

Common Blocks



      none

Procedures Called


      WCS_ROTATE

Author



      Rick Balsano

Modifications/revision Level



      1.1 8/31/93
      2.3 9/15/93 W. Landsman (HSTX) Update quad cube coords, vectorize

Keywords


      2.4 12/29/93 I. Freedman (HSTX) Eliminated LU decomposition
      2.5 1/5/93 I. Freedman (HSTX) Offset keywords / bad point index
      2.6 Dec 94 Compute pole for transformations where the reference
                      pixel is at the native origin W. Landsman (HSTX)
      2.7 May 95 Change internal variable BETA for V4.0 compatibility
      2.8 June 95 Change loop indices from integer to long
      2.9 3/18/96 Change FACE usage for cube projections to match WCSLIB
                      C/FORTRAN software library.
      2.10 02/18/99 Fixed implementation of ARC algorithm
      2.11 June 2003 Update conic projections, add LATPOLE keyword
    2.12 Aug 2003, N.Rich - Fix pre-V5.5 bug from previous update
      2.13 Sep 2003, W. Landsman CTYPE keywords need not be 8 characters
      2.14 Jan 2004, W. Landsman don't modify scalars, fix PARabolic code
      2.15 Feb 2004, W. Landsman Fix AZP and AIR algorithms
      3.0 May 2004 W. Landsman Support extended SIN (=NCP), slant zenithal
                  (SZP), and zenithal polynomial (ZPN) projections, use
                  PV2 keyword vector instead of PROJP1, PROJP2
      3.1 Jul 2005 W.Landsman/C. Markwardt Set unprojectable points in
                  tangent projection to NaN
      3.1.1 Jul 2005 Fixed 3.1 mod to work for scalars
      3.2 Dec 2005 Fixed Airy projection for latitude centered at 90 deg
      3.3 Aug 2007 R. Munoz, W.Landsman Correct treatment of PV1_2 and
                        PV2_2 parameters
      3.4 Oct 2007 Sergey Koposov Support HEALPIX projection
      3.4.1 June 2009 Check for range of validity of ZPN polynomial W.L.
      3.5 May 2012 Benjamin Alan Weaver, Add nonstandard HEALCART
                        projection, Allow map_index to be > 25
      3.5.1 May 2013 W. Landsman Allow GLS as a synonym for SFL
      3.6 Jul 2013 J. P. Leahy added XPH projection, apply polar offsets
                        only for cylindrical & conic projections.
      3.6.1 Dec 2013 W. Landsman Polar offsets done in radians



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