from __future__ import division
import numpy as np
from PyAstronomy.pyaC import pyaErrors as PE
from PyAstronomy import pyasl


class _ZList:
    """
    Calculate the projected distance between the centers of star and planet.

    The resulting values will be stored in the `_zlist` attribute. Additionally,
    the indices belonging to in-transit points will be saved in the `_intrans`
    attribute. Indices pertaining to the occultation (secondary eclipse) are
    available via the `_inocc` attribute.
    These can be used as input to calculate the transit light-curve.

    Parameters
    ----------
    orbit : string
        Either "circular" or "keplerian".
    """

    def _zlistCirc(self, time):
        """
        Calculate projected distance in case of circular orbit.

        Required parameters: per, i, a (assumes transit center at 0)

        Parameters
        ----------
        time : array
            The time points (unit has to be consistent throughout all parameters
            used for calculation).
        """
        # w = circular frequency
        w = 2.0 * np.pi / self["per"]
        # The angle needed to realize the orbit inclination
        alpha = (90.0 - self["i"]) / 180.0 * np.pi
        # Determine the phases (to ensure that the secondary eclipse is not considered)
        phase = time / self["per"]
        phase -= np.floor(phase)

        # Distance between centers
        wt = w * time
        self._zlist = self["a"] * np.sqrt(
            np.sin(wt) ** 2 + np.sin(alpha) ** 2 * np.cos(wt) ** 2
        )

        # In these cases the 'planet' will be in front of the primary
        self._intrans = np.where(
            (np.abs(self._zlist) < (1 + self["p"]))
            & np.logical_or(phase > 0.75, phase < 0.25)
        )[0]

        # Here, the planet is behind the star (occultation)
        self._inocc = np.where(
            (np.abs(self._zlist) < (1 + self["p"]))
            & np.logical_and(phase > 0.25, phase < 0.75)
        )[0]

    def _zlistKep(self, time):
        """
        Calculate the projected, normalized distance of star and planet centers.

        Required parameters: per, i, a, e, w, T0pa, Omega, p
        Additionally requires: collisionCheck

        Note that in this method the line of sight is the -z direction.

        Parameters
        ----------
        time : array
            The time points (unit has to be consistent throughout all
            parameters used for calculation).
        """
        # Assign values to KeplerEllipse
        self._ke.a = self["a"]
        self._ke.e = self["e"]
        self._ke.i = self["i"]
        self._ke.Omega = self["Omega"]
        self._ke.per = self["per"]
        self._ke.tau = self["tau"]
        self._ke.w = self["w"]

        # Initialize the z-list (NaN values will be neglected)
        self._zlist = np.empty(len(time))
        self._zlist[:] = np.NAN
        # Get position of body from Keplerian orbit
        pos = self._ke.xyzPos(time)

        # Default line of sight is in +z direction (i.e., observer
        # located at -z)

        # Calculate projected distance between centers of star and
        # planet sqrt(x**2 + y**2)
        z = np.sqrt(pos[::, 0] ** 2 + pos[::, 1] ** 2)

        # If enabled, check for body collisions
        if self._collisionCheck:
            r = np.sqrt(pos[::, 0] ** 2 + pos[::, 1] ** 2 + pos[::, 2] ** 2)
            indi = np.where(r < 1.0 + self["p"])[0]
            if len(indi) > 0:
                raise (
                    PE.PyAValError(
                        "There is a body collision on this orbit.", where="_ZList"
                    )
                )

        # Determine which values are relevant. In particular, these are those
        # for which the planet is in front of the star (z > 0) and the distance
        # between stellar and planetary distance is lower than 1+p.
        self._intrans = np.where(
            np.logical_and(z <= (1.0 + self["p"]), pos[::, 2] < 0.0)
        )[0]
        self._inocc = np.where(
            np.logical_and(z <= (1.0 + self["p"]), pos[::, 2] > 0.0)
        )[0]

        # Calculate the 'orbit' and store z-values in _zlist
        self._zlist = z

    def __init__(self, orbit, cc=True):
        if orbit == "circular":
            self._calcZList = self._zlistCirc
        elif orbit == "keplerian":
            self._collisionCheck = cc
            self._ke = pyasl.KeplerEllipse(1.0, 1.0)
            self._calcZList = self._zlistKep
