fringe.py

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# This file is part of ip_isr.
#
# Developed for the LSST Data Management System.
# This product includes software developed by the LSST Project
# (https://www.lsst.org).
# See the COPYRIGHT file at the top-level directory of this distribution
# for details of code ownership.
#
# This program is free software: you can redistribute it and/or modify
# it under the terms of the GNU General Public License as published by
# the Free Software Foundation, either version 3 of the License, or
# (at your option) any later version.
#
# This program is distributed in the hope that it will be useful,
# but WITHOUT ANY WARRANTY; without even the implied warranty of
# MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE.  See the
# GNU General Public License for more details.
#
# You should have received a copy of the GNU General Public License
# along with this program.  If not, see <https://www.gnu.org/licenses/>.
 
import numpy
 
import lsst.geom
import lsst.afw.image as afwImage
import lsst.afw.math as afwMath
import lsst.afw.display as afwDisplay
 
from lsst.pipe.base import Task, Struct, timeMethod
from lsst.pex.config import Config, Field, ListField, ConfigField
 
afwDisplay.setDefaultMaskTransparency(75)
 
 
def getFrame():
    """Produce a new frame number each time"""
    getFrame.frame += 1
    return getFrame.frame
 
 
getFrame.frame = 0
 
 
class FringeStatisticsConfig(Config):
    """Options for measuring fringes on an exposure"""
    badMaskPlanes = ListField(dtype=str, default=["SAT"], doc="Ignore pixels with these masks")
    stat = Field(dtype=int, default=int(afwMath.MEDIAN), doc="Statistic to use")
    clip = Field(dtype=float, default=3.0, doc="Sigma clip threshold")
    iterations = Field(dtype=int, default=3, doc="Number of fitting iterations")
    rngSeedOffset = Field(dtype=int, default=0,
                          doc="Offset to the random number generator seed (full seed includes exposure ID)")
 
 
class FringeConfig(Config):
    """Fringe subtraction options"""
    filters = ListField(dtype=str, default=[], doc="Only fringe-subtract these filters")
    num = Field(dtype=int, default=30000, doc="Number of fringe measurements")
    small = Field(dtype=int, default=3, doc="Half-size of small (fringe) measurements (pixels)")
    large = Field(dtype=int, default=30, doc="Half-size of large (background) measurements (pixels)")
    iterations = Field(dtype=int, default=20, doc="Number of fitting iterations")
    clip = Field(dtype=float, default=3.0, doc="Sigma clip threshold")
    stats = ConfigField(dtype=FringeStatisticsConfig, doc="Statistics for measuring fringes")
    pedestal = Field(dtype=bool, default=False, doc="Remove fringe pedestal?")
 
 
class FringeTask(Task):
    """Task to remove fringes from a science exposure
 
    We measure fringe amplitudes at random positions on the science exposure
    and at the same positions on the (potentially multiple) fringe frames
    and solve for the scales simultaneously.
    """
    ConfigClass = FringeConfig
    _DefaultName = 'isrFringe'
 
    def readFringes(self, dataRef, assembler=None):
        """Read the fringe frame(s), and pack data into a Struct
 
        The current implementation assumes only a single fringe frame and
        will have to be updated to support multi-mode fringe subtraction.
 
        This implementation could be optimised by persisting the fringe
        positions and fluxes.
 
        Parameters
        ----------
        dataRef : `daf.butler.butlerSubset.ButlerDataRef`
            Butler reference for the exposure that will have fringing
            removed.
        assembler : `lsst.ip.isr.AssembleCcdTask`, optional
            An instance of AssembleCcdTask (for assembling fringe
            frames).
 
        Returns
        -------
        fringeData : `pipeBase.Struct`
            Struct containing fringe data:
            - ``fringes`` : `lsst.afw.image.Exposure` or `list` thereof
                Calibration fringe files containing master fringe frames.
            - ``seed`` : `int`, optional
                Seed for random number generation.
        """
        try:
            fringe = dataRef.get("fringe", immediate=True)
        except Exception as e:
            raise RuntimeError("Unable to retrieve fringe for %s: %s" % (dataRef.dataId, e))
 
        return self.loadFringes(fringe, assembler)
 
    def loadFringes(self, fringeExp, expId=0, assembler=None):
        """Pack the fringe data into a Struct.
 
        This method moves the struct parsing code into a butler
        generation agnostic handler.
 
        Parameters
        ----------
        fringeExp : `lsst.afw.exposure.Exposure`
            The exposure containing the fringe data.
        expId : `int`, optional
            Exposure id to be fringe corrected, used to set RNG seed.
        assembler : `lsst.ip.isr.AssembleCcdTask`, optional
            An instance of AssembleCcdTask (for assembling fringe
            frames).
 
        Returns
        -------
        fringeData : `pipeBase.Struct`
            Struct containing fringe data:
            - ``fringes`` : `lsst.afw.image.Exposure` or `list` thereof
                Calibration fringe files containing master fringe frames.
            - ``seed`` : `int`, optional
                Seed for random number generation.
        """
        if assembler is not None:
            fringeExp = assembler.assembleCcd(fringeExp)
 
        if expId is None:
            seed = self.config.stats.rngSeedOffset
        else:
            print(f"{self.config.stats.rngSeedOffset} {expId}")
            seed = self.config.stats.rngSeedOffset + expId
 
        # Seed for numpy.random.RandomState must be convertable to a 32 bit unsigned integer
        seed %= 2**32
 
        return Struct(fringes=fringeExp,
                      seed=seed)
 
    @timeMethod
    def run(self, exposure, fringes, seed=None):
        """Remove fringes from the provided science exposure.
 
        Primary method of FringeTask.  Fringes are only subtracted if the
        science exposure has a filter listed in the configuration.
 
        Parameters
        ----------
        exposure : `lsst.afw.image.Exposure`
            Science exposure from which to remove fringes.
        fringes : `lsst.afw.image.Exposure` or `list` thereof
            Calibration fringe files containing master fringe frames.
        seed : `int`, optional
            Seed for random number generation.
 
        Returns
        -------
        solution : `np.array`
            Fringe solution amplitudes for each input fringe frame.
        rms : `float`
            RMS error for the fit solution for this exposure.
        """
        import lsstDebug
        display = lsstDebug.Info(__name__).display
 
        if not self.checkFilter(exposure):
            self.log.info("Filter not found in FringeTaskConfig.filters. Skipping fringe correction.")
            return
 
        if seed is None:
            seed = self.config.stats.rngSeedOffset
        rng = numpy.random.RandomState(seed=seed)
 
        if not hasattr(fringes, '__iter__'):
            fringes = [fringes]
 
        mask = exposure.getMaskedImage().getMask()
        for fringe in fringes:
            fringe.getMaskedImage().getMask().__ior__(mask)
            if self.config.pedestal:
                self.removePedestal(fringe)
 
        positions = self.generatePositions(fringes[0], rng)
        fluxes = numpy.ndarray([self.config.num, len(fringes)])
        for i, f in enumerate(fringes):
            fluxes[:, i] = self.measureExposure(f, positions, title="Fringe frame")
 
        expFringes = self.measureExposure(exposure, positions, title="Science")
        solution, rms = self.solve(expFringes, fluxes)
        self.subtract(exposure, fringes, solution)
        if display:
            afwDisplay.Display(frame=getFrame()).mtv(exposure, title="Fringe subtracted")
        return solution, rms
 
    @timeMethod
    def runDataRef(self, exposure, dataRef, assembler=None):
        """Remove fringes from the provided science exposure.
 
        Retrieve fringes from butler dataRef provided and remove from
        provided science exposure. Fringes are only subtracted if the
        science exposure has a filter listed in the configuration.
 
        Parameters
        ----------
        exposure : `lsst.afw.image.Exposure`
            Science exposure from which to remove fringes.
        dataRef : `daf.persistence.butlerSubset.ButlerDataRef`
            Butler reference to the exposure.  Used to find
            appropriate fringe data.
        assembler : `lsst.ip.isr.AssembleCcdTask`, optional
            An instance of AssembleCcdTask (for assembling fringe
            frames).
 
        Returns
        -------
        solution : `np.array`
            Fringe solution amplitudes for each input fringe frame.
        rms : `float`
            RMS error for the fit solution for this exposure.
        """
        if not self.checkFilter(exposure):
            self.log.info("Filter not found in FringeTaskConfig.filters. Skipping fringe correction.")
            return
        fringeStruct = self.readFringes(dataRef, assembler=assembler)
        return self.run(exposure, **fringeStruct.getDict())
 
    def checkFilter(self, exposure):
        """Check whether we should fringe-subtract the science exposure.
 
        Parameters
        ----------
        exposure : `lsst.afw.image.Exposure`
            Exposure to check the filter of.
 
        Returns
        -------
        needsFringe : `bool`
            If True, then the exposure has a filter listed in the
            configuration, and should have the fringe applied.
        """
        return exposure.getFilter().getName() in self.config.filters
 
    def removePedestal(self, fringe):
        """Remove pedestal from fringe exposure.
 
        Parameters
        ----------
        fringe : `lsst.afw.image.Exposure`
            Fringe data to subtract the pedestal value from.
        """
        stats = afwMath.StatisticsControl()
        stats.setNumSigmaClip(self.config.stats.clip)
        stats.setNumIter(self.config.stats.iterations)
        mi = fringe.getMaskedImage()
        pedestal = afwMath.makeStatistics(mi, afwMath.MEDIAN, stats).getValue()
        self.log.info("Removing fringe pedestal: %f", pedestal)
        mi -= pedestal
 
    def generatePositions(self, exposure, rng):
        """Generate a random distribution of positions for measuring fringe amplitudes.
 
        Parameters
        ----------
        exposure : `lsst.afw.image.Exposure`
            Exposure to measure the positions on.
        rng : `numpy.random.RandomState`
            Random number generator to use.
 
        Returns
        -------
        positions : `numpy.array`
            Two-dimensional array containing the positions to sample
            for fringe amplitudes.
        """
        start = self.config.large
        num = self.config.num
        width = exposure.getWidth() - self.config.large
        height = exposure.getHeight() - self.config.large
        return numpy.array([rng.randint(start, width, size=num),
                            rng.randint(start, height, size=num)]).swapaxes(0, 1)
 
    @timeMethod
    def measureExposure(self, exposure, positions, title="Fringe"):
        """Measure fringe amplitudes for an exposure
 
        The fringe amplitudes are measured as the statistic within a square
        aperture.  The statistic within a larger aperture are subtracted so
        as to remove the background.
 
        Parameters
        ----------
        exposure : `lsst.afw.image.Exposure`
            Exposure to measure the positions on.
        positions : `numpy.array`
            Two-dimensional array containing the positions to sample
            for fringe amplitudes.
        title : `str`, optional
            Title used for debug out plots.
 
        Returns
        -------
        fringes : `numpy.array`
            Array of measured exposure values at each of the positions
            supplied.
        """
        stats = afwMath.StatisticsControl()
        stats.setNumSigmaClip(self.config.stats.clip)
        stats.setNumIter(self.config.stats.iterations)
        stats.setAndMask(exposure.getMaskedImage().getMask().getPlaneBitMask(self.config.stats.badMaskPlanes))
 
        num = self.config.num
        fringes = numpy.ndarray(num)
 
        for i in range(num):
            x, y = positions[i]
            small = measure(exposure.getMaskedImage(), x, y, self.config.small, self.config.stats.stat, stats)
            large = measure(exposure.getMaskedImage(), x, y, self.config.large, self.config.stats.stat, stats)
            fringes[i] = small - large
 
        import lsstDebug
        display = lsstDebug.Info(__name__).display
        if display:
            disp = afwDisplay.Display(frame=getFrame())
            disp.mtv(exposure, title=title)
            if False:
                with disp.Buffering():
                    for x, y in positions:
                        corners = numpy.array([[-1, -1], [1, -1], [1, 1], [-1, 1], [-1, -1]]) + [[x, y]]
                        disp.line(corners*self.config.small, ctype=afwDisplay.GREEN)
                        disp.line(corners*self.config.large, ctype=afwDisplay.BLUE)
 
        return fringes
 
    @timeMethod
    def solve(self, science, fringes):
        """Solve for the scale factors with iterative clipping.
 
        Parameters
        ----------
        science : `numpy.array`
            Array of measured science image values at each of the
            positions supplied.
        fringes : `numpy.array`
            Array of measured fringe values at each of the positions
            supplied.
 
        Returns
        -------
        solution : `np.array`
            Fringe solution amplitudes for each input fringe frame.
        rms : `float`
            RMS error for the fit solution for this exposure.
        """
        import lsstDebug
        doPlot = lsstDebug.Info(__name__).plot
 
        origNum = len(science)
 
        def emptyResult(msg=""):
            """Generate an empty result for return to the user
 
            There are no good pixels; doesn't matter what we return.
            """
            self.log.warn("Unable to solve for fringes: no good pixels%s", msg)
            out = [0]
            if len(fringes) > 1:
                out = out*len(fringes)
            return numpy.array(out), numpy.nan
 
        good = numpy.where(numpy.logical_and(numpy.isfinite(science), numpy.any(numpy.isfinite(fringes), 1)))
        science = science[good]
        fringes = fringes[good]
        oldNum = len(science)
        if oldNum == 0:
            return emptyResult()
 
        # Up-front rejection to get rid of extreme, potentially troublesome values
        # (e.g., fringe apertures that fall on objects).
        good = select(science, self.config.clip)
        for ff in range(fringes.shape[1]):
            good &= select(fringes[:, ff], self.config.clip)
        science = science[good]
        fringes = fringes[good]
        oldNum = len(science)
        if oldNum == 0:
            return emptyResult(" after initial rejection")
 
        for i in range(self.config.iterations):
            solution = self._solve(science, fringes)
            resid = science - numpy.sum(solution*fringes, 1)
            rms = stdev(resid)
            good = numpy.logical_not(abs(resid) > self.config.clip*rms)
            self.log.debug("Iteration %d: RMS=%f numGood=%d", i, rms, good.sum())
            self.log.debug("Solution %d: %s", i, solution)
            newNum = good.sum()
            if newNum == 0:
                return emptyResult(" after %d rejection iterations" % i)
 
            if doPlot:
                import matplotlib.pyplot as plot
                for j in range(fringes.shape[1]):
                    fig = plot.figure(j)
                    fig.clf()
                    try:
                        fig.canvas._tkcanvas._root().lift()  # == Tk's raise
                    except Exception:
                        pass
                    ax = fig.add_subplot(1, 1, 1)
                    adjust = science.copy()
                    others = set(range(fringes.shape[1]))
                    others.discard(j)
                    for k in others:
                        adjust -= solution[k]*fringes[:, k]
                    ax.plot(fringes[:, j], adjust, 'r.')
                    xmin = fringes[:, j].min()
                    xmax = fringes[:, j].max()
                    ymin = solution[j]*xmin
                    ymax = solution[j]*xmax
                    ax.plot([xmin, xmax], [ymin, ymax], 'b-')
                    ax.set_title("Fringe %d: %f" % (j, solution[j]))
                    ax.set_xlabel("Fringe amplitude")
                    ax.set_ylabel("Science amplitude")
                    ax.set_autoscale_on(False)
                    ax.set_xbound(lower=xmin, upper=xmax)
                    ax.set_ybound(lower=ymin, upper=ymax)
                    fig.show()
                while True:
                    ans = input("Enter or c to continue [chp]").lower()
                    if ans in ("", "c",):
                        break
                    if ans in ("p",):
                        import pdb
                        pdb.set_trace()
                    elif ans in ("h", ):
                        print("h[elp] c[ontinue] p[db]")
 
            if newNum == oldNum:
                # Not gaining
                break
            oldNum = newNum
            good = numpy.where(good)
            science = science[good]
            fringes = fringes[good]
 
        # Final solution without rejection
        solution = self._solve(science, fringes)
        self.log.info("Fringe solution: %s RMS: %f Good: %d/%d", solution, rms, len(science), origNum)
        return solution, rms
 
    def _solve(self, science, fringes):
        """Solve for the scale factors.
 
        Parameters
        ----------
        science : `numpy.array`
            Array of measured science image values at each of the
            positions supplied.
        fringes : `numpy.array`
            Array of measured fringe values at each of the positions
            supplied.
 
        Returns
        -------
        solution : `np.array`
            Fringe solution amplitudes for each input fringe frame.
        """
        return afwMath.LeastSquares.fromDesignMatrix(fringes, science,
                                                     afwMath.LeastSquares.DIRECT_SVD).getSolution()
 
    def subtract(self, science, fringes, solution):
        """Subtract the fringes.
 
        Parameters
        ----------
        science : `lsst.afw.image.Exposure`
            Science exposure from which to remove fringes.
        fringes : `lsst.afw.image.Exposure` or `list` thereof
            Calibration fringe files containing master fringe frames.
        solution : `np.array`
            Fringe solution amplitudes for each input fringe frame.
 
        Raises
        ------
        RuntimeError :
            Raised if the number of fringe frames does not match the
            number of measured amplitudes.
        """
        if len(solution) != len(fringes):
            raise RuntimeError("Number of fringe frames (%s) != number of scale factors (%s)" %
                               (len(fringes), len(solution)))
 
        for s, f in zip(solution, fringes):
            science.getMaskedImage().scaledMinus(s, f.getMaskedImage())
 
 
def measure(mi, x, y, size, statistic, stats):
    """Measure a statistic within an aperture
 
    @param mi          MaskedImage to measure
    @param x, y        Center for aperture
    @param size        Size of aperture
    @param statistic   Statistic to measure
    @param stats       StatisticsControl object
    @return Value of statistic within aperture
    """
    bbox = lsst.geom.Box2I(lsst.geom.Point2I(int(x) - size, int(y - size)),
                           lsst.geom.Extent2I(2*size, 2*size))
    subImage = mi.Factory(mi, bbox, afwImage.LOCAL)
    return afwMath.makeStatistics(subImage, statistic, stats).getValue()
 
 
def stdev(vector):
    """Calculate a robust standard deviation of an array of values
 
    @param vector  Array of values
    @return Standard deviation
    """
    q1, q3 = numpy.percentile(vector, (25, 75))
    return 0.74*(q3 - q1)
 
 
def select(vector, clip):
    """Select values within 'clip' standard deviations of the median
 
    Returns a boolean array.
    """
    q1, q2, q3 = numpy.percentile(vector, (25, 50, 75))
    return numpy.abs(vector - q2) < clip*0.74*(q3 - q1)