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# Source code for astropy.coordinates.angle_utilities

    # Licensed under a 3-clause BSD style license - see LICENSE.rst
    """
    This module contains utility functions for working with angles. These are both
    used internally in astropy.coordinates.angles, and of possible
    """

    __all__ = [
        "angular_separation",
        "position_angle",
        "offset_by",
        "golden_spiral_grid",
        "uniform_spherical_random_surface",
        "uniform_spherical_random_volume",
    ]

    # Third-party
    import numpy as np

    # Astropy
    import astropy.units as u
    from astropy.coordinates.representation import (
        SphericalRepresentation,
        UnitSphericalRepresentation,
    )

    _TWOPI = 2 * np.pi

    def angular_separation(lon1, lat1, lon2, lat2):
        """
        Angular separation between two points on a sphere.

        Parameters
        ----------
        lon1, lat1, lon2, lat2 : `~astropy.coordinates.Angle`, `~astropy.units.Quantity` or float
            Longitude and latitude of the two points. Quantities should be in
            angular units; floats in radians.

        Returns
        -------
        angular separation : `~astropy.units.Quantity` ['angle'] or float
            Type depends on input; ``Quantity`` in angular units, or float in
            radians.

        Notes
        -----
        The angular separation is calculated using the Vincenty formula [1]_,
        which is slightly more complex and computationally expensive than
        some alternatives, but is stable at at all distances, including the
        poles and antipodes.

        .. [1] https://en.wikipedia.org/wiki/Great-circle_distance
        """

        sdlon = np.sin(lon2 - lon1)
        cdlon = np.cos(lon2 - lon1)
        slat1 = np.sin(lat1)
        slat2 = np.sin(lat2)
        clat1 = np.cos(lat1)
        clat2 = np.cos(lat2)

        num1 = clat2 * sdlon
        num2 = clat1 * slat2 - slat1 * clat2 * cdlon
        denominator = slat1 * slat2 + clat1 * clat2 * cdlon

        return np.arctan2(np.hypot(num1, num2), denominator)

    def position_angle(lon1, lat1, lon2, lat2):
        """
        Position Angle (East of North) between two points on a sphere.

        Parameters
        ----------
        lon1, lat1, lon2, lat2 : `~astropy.coordinates.Angle`, `~astropy.units.Quantity` or float
            Longitude and latitude of the two points. Quantities should be in
            angular units; floats in radians.

        Returns
        -------
        pa : `~astropy.coordinates.Angle`
            The (positive) position angle of the vector pointing from position 1 to
            position 2.  If any of the angles are arrays, this will contain an array
            following the appropriate `numpy` broadcasting rules.

        """
        from .angles import Angle

        deltalon = lon2 - lon1
        colat = np.cos(lat2)

        x = np.sin(lat2) * np.cos(lat1) - colat * np.sin(lat1) * np.cos(deltalon)
        y = np.sin(deltalon) * colat

        return Angle(np.arctan2(y, x), u.radian).wrap_at(360 * u.deg)

    def offset_by(lon, lat, posang, distance):
        """
        Point with the given offset from the given point.

        Parameters
        ----------
        lon, lat, posang, distance : `~astropy.coordinates.Angle`, `~astropy.units.Quantity` or float
            Longitude and latitude of the starting point,
            position angle and distance to the final point.
            Quantities should be in angular units; floats in radians.
            Polar points at lat= +/-90 are treated as limit of +/-(90-epsilon) and same lon.

        Returns
        -------
        lon, lat : `~astropy.coordinates.Angle`
            The position of the final point.  If any of the angles are arrays,
            these will contain arrays following the appropriate `numpy` broadcasting rules.
            0 <= lon < 2pi.
        """
        from .angles import Angle

        # Calculations are done using the spherical trigonometry sine and cosine rules
        # of the triangle A at North Pole,   B at starting point,   C at final point
        # with angles     A (change in lon), B (posang),            C (not used, but negative reciprocal posang)
        # with sides      a (distance),      b (final co-latitude), c (starting colatitude)
        # B, a, c are knowns; A and b are unknowns
        # https://en.wikipedia.org/wiki/Spherical_trigonometry

        cos_a = np.cos(distance)
        sin_a = np.sin(distance)
        cos_c = np.sin(lat)
        sin_c = np.cos(lat)
        cos_B = np.cos(posang)
        sin_B = np.sin(posang)

        # cosine rule: Know two sides: a,c and included angle: B; get unknown side b
        cos_b = cos_c * cos_a + sin_c * sin_a * cos_B
        # sin_b = np.sqrt(1 - cos_b**2)
        # sine rule and cosine rule for A (using both lets arctan2 pick quadrant).
        # multiplying both sin_A and cos_A by x=sin_b * sin_c prevents /0 errors
        # at poles.  Correct for the x=0 multiplication a few lines down.
        # sin_A/sin_a == sin_B/sin_b    # Sine rule
        xsin_A = sin_a * sin_B * sin_c
        # cos_a == cos_b * cos_c + sin_b * sin_c * cos_A  # cosine rule
        xcos_A = cos_a - cos_b * cos_c

        A = Angle(np.arctan2(xsin_A, xcos_A), u.radian)
        # Treat the poles as if they are infinitesimally far from pole but at given lon
        small_sin_c = sin_c < 1e-12
        if small_sin_c.any():
            # For south pole (cos_c = -1), A = posang; for North pole, A=180 deg - posang
            A_pole = (90 * u.deg + cos_c * (90 * u.deg - Angle(posang, u.radian))).to(u.rad)
            if A.shape:
                # broadcast to ensure the shape is like that of A, which is also
                # affected by the (possible) shapes of lat, posang, and distance.
                small_sin_c = np.broadcast_to(small_sin_c, A.shape)
                A[small_sin_c] = A_pole[small_sin_c]
            else:
                A = A_pole

        outlon = (Angle(lon, u.radian) + A).wrap_at(360.0 * u.deg).to(u.deg)
        outlat = Angle(np.arcsin(cos_b), u.radian).to(u.deg)

        return outlon, outlat

    def golden_spiral_grid(size):
        """Generate a grid of points on the surface of the unit sphere using the
        Fibonacci or Golden Spiral method.

        .. seealso::

            `Evenly distributing points on a sphere <https://stackoverflow.com/questions/9600801/evenly-distributing-n-points-on-a-sphere>`_

        Parameters
        ----------
        size : int
            The number of points to generate.

        Returns
        -------
        rep : `~astropy.coordinates.UnitSphericalRepresentation`
            The grid of points.
        """
        golden_r = (1 + 5**0.5) / 2

        grid = np.arange(0, size, dtype=float) + 0.5
        lon = _TWOPI / golden_r * grid * u.rad
        lat = np.arcsin(1 - 2 * grid / size) * u.rad

        return UnitSphericalRepresentation(lon, lat)

    def uniform_spherical_random_surface(size=1):
        """Generate a random sampling of points on the surface of the unit sphere.

        Parameters
        ----------
        size : int
            The number of points to generate.

        Returns
        -------
        rep : `~astropy.coordinates.UnitSphericalRepresentation`
            The random points.
        """

        rng = np.random  # can maybe switch to this being an input later - see #11628

        lon = rng.uniform(0, _TWOPI, size) * u.rad
        lat = np.arcsin(rng.uniform(-1, 1, size=size)) * u.rad

        return UnitSphericalRepresentation(lon, lat)

    def uniform_spherical_random_volume(size=1, max_radius=1):
        """Generate a random sampling of points that follow a uniform volume
        density distribution within a sphere.

        Parameters
        ----------
        size : int
            The number of points to generate.
        max_radius : number, quantity-like, optional
            A dimensionless or unit-ful factor to scale the random distances.

        Returns
        -------
        rep : `~astropy.coordinates.SphericalRepresentation`
            The random points.
        """
        rng = np.random  # can maybe switch to this being an input later - see #11628

        usph = uniform_spherical_random_surface(size=size)

        r = np.cbrt(rng.uniform(size=size)) * u.Quantity(max_radius, copy=False)
        return SphericalRepresentation(usph.lon, usph.lat, r)

    from astropy.coordinates import angle_formats

    # # below here can be deleted in v5.0
    from astropy.utils.decorators import deprecated

    __old_angle_utilities_funcs = [
        "check_hms_ranges",
        "degrees_to_dms",
        "degrees_to_string",
        "dms_to_degrees",
        "format_exception",
        "hms_to_degrees",
        "hms_to_dms",
        "hms_to_hours",
        "hms_to_radians",
        "hours_to_decimal",
        "hours_to_hms",
        "hours_to_radians",
        "hours_to_string",
        "parse_angle",
        "radians_to_degrees",
        "radians_to_dms",
        "radians_to_hms",
        "radians_to_hours",
        "sexagesimal_to_string",
    ]
    for funcname in __old_angle_utilities_funcs:
        vars()[funcname] = deprecated(
            name="astropy.coordinates.angle_utilities." + funcname,
            alternative="astropy.coordinates.angle_formats." + funcname,
            since="v4.3",
        )(getattr(angle_formats, funcname))