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Merge pull request #176 from lsst/tickets/DM-23694
DM-23694: Create script for producing distortion model from Jointcal output
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# This file is part of jointcal. | ||
# | ||
# 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/>. | ||
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"""Code to convert jointcal's output WCS models to distortion maps that can be | ||
used by afw CameraGeom. | ||
""" | ||
import numpy as np | ||
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from lsst.afw import cameraGeom | ||
import lsst.afw.geom | ||
import astshim as ast | ||
import lsst.log | ||
from lsst.geom import SpherePoint, Point2D, radians | ||
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class CameraModel: | ||
"""Convert a jointcal `~lsst.afw.geom.SkyWcs` into a distortion model and | ||
detector positions (TODO) that can be used by `~lsst.afw.cameraGeom`. | ||
Because this code only operates on the WCS, it is independent of the | ||
format of the persisted output (e.g. gen2 separate files vs. gen3 bundled | ||
visits). | ||
Parameters | ||
---------- | ||
wcsList : `list` [`lsst.afw.geom.SkyWcs`] | ||
The WCS to use to compute the distortion model from, preferably from | ||
multiple visits on the same tract. | ||
detectors : `list` [`int`] | ||
Detector ids that correspond one-to-one with ``wcsList``. | ||
camera : `lsst.afw.cameraGeom.Camera` | ||
The camera these WCS were fit for. | ||
n : `int` | ||
Number of points to compute the pixel scale at, along the +y axis. | ||
""" | ||
def __init__(self, wcsList, detectors, camera, n=100): | ||
self.wcsList = wcsList | ||
self.camera = camera | ||
self.detectors = detectors | ||
self.maxFocalRadius = self.camera.computeMaxFocalPlaneRadius() | ||
self.n = n | ||
# the computed radius and pixel scales | ||
self.fieldAngle = None # degrees | ||
self.radialScale = None # arcsec | ||
self.tangentialScale = None # arcsec | ||
# the computed values for every input wcs | ||
self.fieldAngles = None | ||
self.radialScales = None | ||
self.tangentialScales = None | ||
self.fieldAngleStd = None | ||
self.radialScaleStd = None | ||
self.tangentialScaleStd = None | ||
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self.log = lsst.log.Log.getLogger("jointcal.cameraGeom.CameraModel") | ||
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def computeDistortionModel(self): | ||
"""Calculate the afw cameraGeom distortion model to be included in an | ||
on-disk camera model. | ||
PLACEHOLDER: This may be as simple as running `computePixelScale` and | ||
then doing a numpy polynomial fit to it for the cameraGeom input. | ||
However, we need to check details of how that distortion model is | ||
stored in a Camera. | ||
e.g.: np.polyfit(self.fieldAngle, self.radialScale, poly_degree)) | ||
""" | ||
raise NotImplementedError("not yet!") | ||
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def computePixelScale(self): | ||
"""Compute the radial and tangential pixel scale by averaging over | ||
multiple jointcal WCS models. | ||
Also computes the standard deviation and logs any WCS that are | ||
significant outliers. | ||
The calculations are stored in the ``fieldAngle[s]``, | ||
``radialScale[s]``, and ``tangentialScale[s]`` member variables. | ||
""" | ||
self.fieldAngles = [] | ||
self.radialScales = [] | ||
self.tangentialScales = [] | ||
for id, wcs in zip(self.detectors, self.wcsList): | ||
fieldAngle, radial, tangential = self._computeDetectorPixelScale(id, wcs) | ||
self.fieldAngles.append(fieldAngle) | ||
self.radialScales.append(radial) | ||
self.tangentialScales.append(tangential) | ||
# TODO: For now, don't worry about small differences in the computed | ||
# field angles vs. their respective radial/tangential scales, just | ||
# assume all fieldAngle positions are "close enough" and warn if not. | ||
self.fieldAngle = np.mean(self.fieldAngles, axis=0) | ||
self.fieldAngleStd = np.std(self.fieldAngles, axis=0) | ||
if self.fieldAngleStd.max() > 1e-4: | ||
self.log.warn("Large stddev in computed field angles between visits (max: %s degree).", | ||
self.fieldAngleStd.max()) | ||
# import os; print(os.getpid()); import ipdb; ipdb.set_trace(); | ||
self.radialScale = np.mean(self.radialScales, axis=0) | ||
self.radialScaleStd = np.std(self.radialScales, axis=0) | ||
if self.radialScaleStd.max() > 1e-4: | ||
self.log.warn("Large stddev in computed radial scales between visits (max: %s arcsec).", | ||
self.radialScaleStd.max()) | ||
self.tangentialScale = np.mean(self.tangentialScales, axis=0) | ||
self.tangentialScaleStd = np.std(self.tangentialScales, axis=0) | ||
if self.tangentialScaleStd.max() > 1e-4: | ||
self.log.warn("Large stddev in computed tangential scales between visits (max: %s arcsec).", | ||
self.tangentialScaleStd.max()) | ||
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def computeCameraPixelScale(self, detector_id=30): | ||
"""Compute the radial and tangential pixel scales using the distortion | ||
model supplied with the camera. | ||
This is designed to be directly comparable with the results of | ||
`~CameraModel.computePixelScale`. | ||
Parameters | ||
---------- | ||
detector_id: `int` | ||
Detector identifier for the detector_id to use for the calculation. | ||
Returns | ||
------- | ||
fieldAngle : `numpy.ndarray` | ||
Field angles in degrees. | ||
radialScale : `numpy.ndarray` | ||
Radial direction pixel scales in arcseconds/pixel. | ||
tangentialScale : `numpy.ndarray` | ||
Tangential direction pixel scales in arcseconds/pixel. | ||
""" | ||
# Make a trivial SkyWcs to get a field angle->sky transform from. | ||
iwcToSkyWcs = lsst.afw.geom.makeSkyWcs(Point2D(0, 0), SpherePoint(0, 0, radians), | ||
lsst.afw.geom.makeCdMatrix(1.0 * radians, 0 * radians, True)) | ||
iwcToSkyMap = iwcToSkyWcs.getFrameDict().getMapping("PIXELS", "SKY") | ||
skyFrame = iwcToSkyWcs.getFrameDict().getFrame("SKY") | ||
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# Extract the transforms that are defined just on the camera. | ||
pixSys = self.camera[detector_id].makeCameraSys(cameraGeom.PIXELS) | ||
pixelsToFocal = self.camera.getTransform(pixSys, cameraGeom.FOCAL_PLANE) | ||
focalToField = self.camera.getTransform(cameraGeom.FOCAL_PLANE, cameraGeom.FIELD_ANGLE) | ||
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# Build a SkyWcs that combines each of the above components. | ||
pixelFrame = ast.Frame(2, "Domain=PIXELS") | ||
focalFrame = ast.Frame(2, "Domain=FOCAL") | ||
iwcFrame = ast.Frame(2, "Domain=IWC") | ||
frameDict = ast.FrameDict(pixelFrame) | ||
frameDict.addFrame("PIXELS", pixelsToFocal.getMapping(), focalFrame) | ||
frameDict.addFrame("FOCAL", focalToField.getMapping(), iwcFrame) | ||
frameDict.addFrame("IWC", iwcToSkyMap, skyFrame) | ||
wcs = lsst.afw.geom.SkyWcs(frameDict) | ||
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return self._computeDetectorPixelScale(detector_id, wcs) | ||
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def _computeDetectorPixelScale(self, detector_id, wcs): | ||
"""Compute pixel scale in radial and tangential directions as a | ||
function of field angle. | ||
Parameters | ||
---------- | ||
detector_id: `int` | ||
Detector identifier for the detector of this wcs. | ||
wcs : `lsst.afw.geom.SkyWcs` | ||
Full focal-plane model to compute pixel scale on. | ||
Returns | ||
------- | ||
fieldAngle : `numpy.ndarray` | ||
Field angles in degrees. | ||
radialScale : `numpy.ndarray` | ||
Radial direction pixel scales in arcseconds/pixel. | ||
tangentialScale : `numpy.ndarray` | ||
Tangential direction pixel scales in arcseconds/pixel. | ||
Notes | ||
----- | ||
Pixel scales are calculated from finite differences only along the +y | ||
focal plane direction. | ||
""" | ||
focalToSky = wcs.getFrameDict().getMapping('FOCAL', 'SKY') | ||
mmPerPixel = self.camera[detector_id].getPixelSize() | ||
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focalToPixels = wcs.getFrameDict().getMapping('FOCAL', 'PIXELS') | ||
trans = wcs.getTransform() # Pixels to Sky as Point2d -> SpherePoint | ||
boresight = trans.applyForward(Point2D(focalToPixels.applyForward([0, 0]))) | ||
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rs = np.linspace(0, self.maxFocalRadius, self.n) # focal plane units | ||
fieldAngle = np.zeros_like(rs) | ||
radialScale = np.zeros_like(rs) | ||
tangentialScale = np.zeros_like(rs) | ||
for i, r in enumerate(rs): | ||
# point on the sky at position r along the focal plane +y axis | ||
sp1 = SpherePoint(*focalToSky.applyForward(Point2D([0, r])), radians) | ||
# point on the sky one pixel further along the focal plane +y axis | ||
sp2 = SpherePoint(*focalToSky.applyForward(Point2D([0, r + mmPerPixel.getY()])), radians) | ||
# point on the sky one pixel off of the focal plane +y axis at r | ||
sp3 = SpherePoint(*focalToSky.applyForward(Point2D([mmPerPixel.getX(), r])), radians) | ||
fieldAngle[i] = boresight.separation(sp1).asDegrees() | ||
radialScale[i] = sp1.separation(sp2).asArcseconds() | ||
tangentialScale[i] = sp1.separation(sp3).asArcseconds() | ||
return fieldAngle, radialScale, tangentialScale |
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