casa
5.7.0-16
|
Polarimetric analysis of images. More...
#include <ImagePolarimetry.h>
Public Types | |
enum | StokesTypes { I, Q, U, V } |
casacore::Stokes types More... | |
Public Member Functions | |
ImagePolarimetry (const casacore::ImageInterface< casacore::Float > &image) | |
Constructor. More... | |
ImagePolarimetry (const ImagePolarimetry &other) | |
Copy constructor (reference semantics) More... | |
~ImagePolarimetry () | |
Destructor. More... | |
ImagePolarimetry & | operator= (const ImagePolarimetry &other) |
Assignment operator (reference semantics) More... | |
void | summary (casacore::LogIO &os) const |
Summary. More... | |
SPCIIF | imageInterface () const |
Get the casacore::ImageInterface pointer of the construction image Don't delete it ! More... | |
casacore::CoordinateSystem | coordinates () const |
Get the casacore::CoordinateSystem of the construction image. More... | |
casacore::IPosition | shape () const |
Get the shape of the construction image. More... | |
casacore::Bool | isMasked () const |
Is the construction image masked ? More... | |
casacore::IPosition | singleStokesShape (casacore::CoordinateSystem &cSys, casacore::Stokes::StokesTypes type) const |
Get the shape and casacore::CoordinateSystem of an image for a single Stokes pixel. More... | |
casacore::ImageExpr < casacore::Complex > | complexLinearPolarization () |
Complex linear polarization. More... | |
casacore::ImageExpr < casacore::Complex > | complexFractionalLinearPolarization () |
casacore::Complex fractional linear polarization More... | |
casacore::ImageExpr < casacore::Float > | stokesI () const |
Get the Stokes I image and the standard deviation of the I image. More... | |
casacore::Float | sigmaStokesI (casacore::Float clip=10.0) |
casacore::ImageExpr < casacore::Float > | stokesQ () const |
Get the casacore::Stokes Q image and the standard deviation of the Q image. More... | |
casacore::Float | sigmaStokesQ (casacore::Float clip=10.0) |
casacore::ImageExpr < casacore::Float > | stokesU () const |
Get the casacore::Stokes U image and the standard deviation of the U image. More... | |
casacore::Float | sigmaStokesU (casacore::Float clip=10.0) |
casacore::ImageExpr < casacore::Float > | stokesV () const |
Get the casacore::Stokes V image and the standard deviation of the V image. More... | |
casacore::Float | sigmaStokesV (casacore::Float clip=10.0) |
casacore::ImageExpr < casacore::Float > | stokes (ImagePolarimetry::StokesTypes index) const |
Get the specified casacore::Stokes image and the standard deviation of the image. More... | |
casacore::Float | sigmaStokes (ImagePolarimetry::StokesTypes index, casacore::Float clip=10.0) |
casacore::Float | sigma (casacore::Float clip=10.0) |
Get the best estimate of the statistical noise. More... | |
casacore::Float | sigmaLinPolInt (casacore::Float clip=10.0, casacore::Float sigma=-1.0) |
Get the linearly polarized intensity image and its standard deviation. More... | |
casacore::ImageExpr < casacore::Float > | totPolInt (casacore::Bool debias, casacore::Float clip=10.0, casacore::Float sigma=-1.0) |
Get the total polarized intensity (from whatever combination of Q, U, and V the construction image has) image and its error (standard deviation). More... | |
casacore::Float | sigmaTotPolInt (casacore::Float clip=10.0, casacore::Float sigma=-1.0) |
casacore::ImageExpr < casacore::Float > | linPolPosAng (casacore::Bool radians) const |
Get linearly polarized position angle (degrees or radians) image and error (standard deviation). More... | |
casacore::ImageExpr < casacore::Float > | sigmaLinPolPosAng (casacore::Bool radians, casacore::Float clip=10.0, casacore::Float sigma=-1.0) |
casacore::ImageExpr < casacore::Float > | fracLinPol (casacore::Bool debias, casacore::Float clip=10.0, casacore::Float sigma=-1.0) |
Get fractional linear polarization image and error (standard deviation). More... | |
casacore::ImageExpr < casacore::Float > | sigmaFracLinPol (casacore::Float clip=10.0, casacore::Float sigma=-1.0) |
casacore::ImageExpr < casacore::Float > | fracTotPol (casacore::Bool debias, casacore::Float clip=10.0, casacore::Float sigma=-1.0) |
Get Fractional total polarization and error (standard deviation) var is the standard deviation of the thermal noise. More... | |
casacore::ImageExpr < casacore::Float > | sigmaFracTotPol (casacore::Float clip=10.0, casacore::Float sigma=-1.0) |
void | fourierRotationMeasure (casacore::ImageInterface< casacore::Complex > &pol, casacore::Bool zeroZeroLag) |
Fourier Rotation Measure. More... | |
casacore::IPosition | rotationMeasureShape (casacore::CoordinateSystem &cSys, casacore::Int &frequencyAxis, casacore::Int &stokesAxis, casacore::LogIO &os, casacore::Int spectralAxis=-1) const |
This function is used in concert with the rotationMeasure function. More... | |
casacore::IPosition | positionAngleShape (casacore::CoordinateSystem &cSys, casacore::Int &frequencyAxis, casacore::Int &stokesAxis, casacore::LogIO &os, casacore::Int spectralAxis=-1) const |
This function is used in concert with the rotationMeasure function. More... | |
void | rotationMeasure (casacore::ImageInterface< casacore::Float > *&rmPtr, casacore::ImageInterface< casacore::Float > *&rmErrPtr, casacore::ImageInterface< casacore::Float > *&pa0Ptr, casacore::ImageInterface< casacore::Float > *&pa0ErrPtr, casacore::ImageInterface< casacore::Float > *&nTurns, casacore::ImageInterface< casacore::Float > *&rChiSqPtr, casacore::Int spectralAxis, casacore::Float rmMax, casacore::Float maxPaErr=1.0e30, casacore::Float sigma=-1.0, casacore::Float rmFg=0.0, casacore::Bool showProgress=false) |
This function applies a traditional (i.e. More... | |
Static Public Member Functions | |
static casacore::ImageExpr < casacore::Float > | depolarizationRatio (const casacore::ImageInterface< casacore::Float > &im1, const casacore::ImageInterface< casacore::Float > &im2, casacore::Bool debias, casacore::Float clip=10.0, casacore::Float sigma=-1.0) |
Depolarization ratio image and error. More... | |
static casacore::ImageExpr < casacore::Float > | sigmaDepolarizationRatio (const casacore::ImageInterface< casacore::Float > &im1, const casacore::ImageInterface< casacore::Float > &im2, casacore::Bool debias, casacore::Float clip=10.0, casacore::Float sigma=-1.0) |
Static Private Member Functions | |
static void | _checkBeams (const ImagePolarimetry &im1, const ImagePolarimetry &im2, const casacore::Vector< StokesTypes > &stokes) |
Private Attributes | |
SPCIIF | _image |
casacore::LinearFitSVD < casacore::Float > * | _fitter |
const casacore::ImageInterface<casacore::Float>* _image; More... | |
casacore::Float | _oldClip |
casacore::PtrBlock < casacore::ImageInterface < casacore::Float > * > | _stokes |
These blocks are always size 4, with IQUV in slots 0,1,2,3 If your image is IV only, they still use slots 0 and 3. More... | |
casacore::PtrBlock < casacore::LatticeStatistics < casacore::Float > * > | _stokesStats |
casacore::Matrix< casacore::Bool > | _beamsEqMat |
Static Private Attributes | |
static const map< StokesTypes, casacore::String > | polMap |
Polarimetric analysis of images.
Public interface
Polarimetric analysis of Images
This class provides polarimetric image analysis capability. It takes an image with a casacore::Stokes axis (some combination of IQUV is needed) as its input.
Many functions return casacore::ImageExpr objects. These are read-only images.
Sometimes the standard deviation of the noise is needed. This is for debiasing polarized intensity images or working out error images. By default it is worked out for you with a clipped mean algorithm. However, you can provide sigma if you know it accurately. It should be the standard deviation of the noise in the absence of signal. You won't measure that very well from casacore::Stokes I if it is dynamic range limited. Better to get it from V or Q or U. When this class needs the standard deviation of the noise, it will try and get it from V or Q and U and finally I.
However, note that the functions sigmaStokes{I,Q,U,V} DO return the standard deviation of the noise for that specific casacore::Stokes type.
The ImageExpr objects returned have the brightness units and ImageInfo set. The MiscInfo (a permanent record) and logSink are not set.
Basic image analysis capability
Definition at line 109 of file ImagePolarimetry.h.
casa::ImagePolarimetry::ImagePolarimetry | ( | const casacore::ImageInterface< casacore::Float > & | image | ) |
Constructor.
The input image must have a Stokes axis with some subset of I,Q,U, and V
casa::ImagePolarimetry::ImagePolarimetry | ( | const ImagePolarimetry & | other | ) |
Copy constructor (reference semantics)
casa::ImagePolarimetry::~ImagePolarimetry | ( | ) |
Destructor.
|
private |
|
staticprivate |
|
private |
|
private |
|
private |
|
private |
Delete all private pointers.
|
private |
|
private |
For traiditional RM approach, give output a mask if possible.
|
private |
Change the Stokes Coordinate for the given float image to be of the specified Stokes type.
|
private |
|
private |
Change the casacore::Stokes casacore::Coordinate for the given complex image to be of the specified casacore::Stokes type.
|
private |
Change the time coordinate to be rotation measure.
|
private |
Find the central frequency from the given spectral coordinate.
|
private |
FInd frequency axis.
|
private |
Fit the spectrum of position angles to find the rotation measure via Leahy algorithm.
|
private |
Find the spectral coordinate.
|
private |
Find the casacore::Stokes in the construction image and assign pointers.
|
private |
So we have Q and U ? Excpetion if not.
|
private |
Make a LEN for the give types of polarized intensity.
|
private |
Make an IE for the specified Stokes.
|
private |
Make a casacore::SubImage from the construction image for the specified pixel along the specified pixel axis.
|
private |
Least squares fit to find RM from position angles.
|
private |
Fit the spectrum of position angles to find the rotation measure via Leahy algorithm for primary (n>2) points.
|
private |
Fit the spectrum of position angles to find the rotation measure via Leahy algorithm for supplementary (n==2) points.
|
private |
|
private |
|
private |
|
private |
Find the standard deviation for the Stokes image specified by the integer index.
|
private |
Return I, Q, U or V for specified integer index (0-3)
|
private |
Return I, Q, U or V for specified integer index (0-3)
|
private |
Subtract profile mean from image.
casacore::ImageExpr<casacore::Complex> casa::ImagePolarimetry::complexFractionalLinearPolarization | ( | ) |
casacore::Complex fractional linear polarization
casacore::ImageExpr<casacore::Complex> casa::ImagePolarimetry::complexLinearPolarization | ( | ) |
Complex linear polarization.
|
inline |
Get the casacore::CoordinateSystem of the construction image.
Definition at line 139 of file ImagePolarimetry.h.
References _image.
|
static |
Depolarization ratio image and error.
Requires two images hence static functions.
void casa::ImagePolarimetry::fourierRotationMeasure | ( | casacore::ImageInterface< casacore::Complex > & | pol, |
casacore::Bool | zeroZeroLag | ||
) |
Fourier Rotation Measure.
The output image is the complex polarization (Q + iU) with the spectral axis replaced by a RotationMeasure axis. The appropriate shape and casacore::CoordinateSystem must be obtained with function singleStokesShape (ask for type STokes::Plinear). Howeverm this function will replace the casacore::SpectralCoordinate by a LinearCoordinate describing the Rotation Measure. casacore::ImageInfo, and Units are copied to the output. MiscInfo and history are not. If the output has a mask, and the input is masked, the mask is copied. If the output has a mask, it should already have been initialized to true
casacore::ImageExpr<casacore::Float> casa::ImagePolarimetry::fracLinPol | ( | casacore::Bool | debias, |
casacore::Float | clip = 10.0 , |
||
casacore::Float | sigma = -1.0 |
||
) |
Get fractional linear polarization image and error (standard deviation).
If wish to debias the image, you can either provide sigma
(the standard deviation of the termal noise) or if sigma
is non-positive, it will be worked out for you with a clipped mean algorithm.
casacore::ImageExpr<casacore::Float> casa::ImagePolarimetry::fracTotPol | ( | casacore::Bool | debias, |
casacore::Float | clip = 10.0 , |
||
casacore::Float | sigma = -1.0 |
||
) |
Get Fractional total polarization and error (standard deviation) var
is the standard deviation of the thermal noise.
If sigma
is non-positive, it will be worked out for you with a clipped mean algorithm.
|
inline |
Get the casacore::ImageInterface pointer of the construction image Don't delete it !
Definition at line 134 of file ImagePolarimetry.h.
References _image.
Referenced by casa::ImagePol::getImage().
|
inline |
Is the construction image masked ?
Definition at line 149 of file ImagePolarimetry.h.
References _image.
casacore::ImageExpr<casacore::Float> casa::ImagePolarimetry::linPolPosAng | ( | casacore::Bool | radians | ) | const |
Get linearly polarized position angle (degrees or radians) image and error (standard deviation).
If you provide sigma
it is the standard deviation of the termal noise. If sigma
is non-positive, it will be worked out for you with a clipped mean algorithm.
ImagePolarimetry& casa::ImagePolarimetry::operator= | ( | const ImagePolarimetry & | other | ) |
Assignment operator (reference semantics)
casacore::IPosition casa::ImagePolarimetry::positionAngleShape | ( | casacore::CoordinateSystem & | cSys, |
casacore::Int & | frequencyAxis, | ||
casacore::Int & | stokesAxis, | ||
casacore::LogIO & | os, | ||
casacore::Int | spectralAxis = -1 |
||
) | const |
This function is used in concert with the rotationMeasure function.
It tells you what the shape of the output Position Angle image should be, and gives you its CoordinateSystem. Because the ImagePolarimetry construction image may house the frequencies coordinate description in a Spectral, Tabular or Linear coordinate, you may explicitly specify which axis is the Spectral axis (spectralAxis). By default, it tries to find the SpectralCoordinate. If there is none, it will look for Tabular or Linear coordinates with a "FREQ" label.
void casa::ImagePolarimetry::rotationMeasure | ( | casacore::ImageInterface< casacore::Float > *& | rmPtr, |
casacore::ImageInterface< casacore::Float > *& | rmErrPtr, | ||
casacore::ImageInterface< casacore::Float > *& | pa0Ptr, | ||
casacore::ImageInterface< casacore::Float > *& | pa0ErrPtr, | ||
casacore::ImageInterface< casacore::Float > *& | nTurns, | ||
casacore::ImageInterface< casacore::Float > *& | rChiSqPtr, | ||
casacore::Int | spectralAxis, | ||
casacore::Float | rmMax, | ||
casacore::Float | maxPaErr = 1.0e30 , |
||
casacore::Float | sigma = -1.0 , |
||
casacore::Float | rmFg = 0.0 , |
||
casacore::Bool | showProgress = false |
||
) |
This function applies a traditional (i.e.
non-Fourier) Rotation Measure algorithm (Leahy et al, A&A, 156, 234) approach. For the RM images you must get the shape and CoordinateSYstem from function rotationMeasureShape. For the position angle images, use function singleStokesShape. Null pointer ImageInterface objects are not accessed so you can select which output images you want. Any output images not masked will be given a mask. The position angles are all in degrees. The RM images in rad/m/m. ImageInfo and Units, are copied to the output. MiscInfo and history are not. You specify which axis houses the frequencies, the noise level of Q and U if you know it (by default it is worked out for you) for error images, the value of the foreground RM if you know it (helps for unwinding ambiguity), the absolute maximum RM it should solve for, and the maximum error in the position angle that should be allowed. The state of the plotter should be set by the caller (e.g. character size, number of plots in x and y etc).
casacore::IPosition casa::ImagePolarimetry::rotationMeasureShape | ( | casacore::CoordinateSystem & | cSys, |
casacore::Int & | frequencyAxis, | ||
casacore::Int & | stokesAxis, | ||
casacore::LogIO & | os, | ||
casacore::Int | spectralAxis = -1 |
||
) | const |
This function is used in concert with the rotationMeasure function.
It tells you what the shape of the output RM image should be, and gives you its CoordinateSystem. Because the ImagePolarimetry construction image may house the frequencies coordinate description in a Spectral, Tabular or Linear coordinate, you may explicitly specify which axis is the Spectral axis (spectralAxis). By default, it tries to find the SpectralCoordinate. If there is none, it will look for Tabular or Linear coordinates with a "FREQ" label. It returns to you the frequencyAxis (i.e. the one it is concluded houses the frequency spectrum) and the stokesAxis that it finds.
|
inline |
Get the shape of the construction image.
Definition at line 144 of file ImagePolarimetry.h.
References _image.
casacore::Float casa::ImagePolarimetry::sigma | ( | casacore::Float | clip = 10.0 | ) |
Get the best estimate of the statistical noise.
This gives you the standard deviation with outliers from the mean clipped first. The idea is to not be confused by source or dynamic range issues. Generally Stokes V is empty of sources (not always), then Q and U are generally less bright than I. So this function first tries V, then Q and U and lastly I to give you its noise estimate
|
static |
casacore::ImageExpr<casacore::Float> casa::ImagePolarimetry::sigmaFracLinPol | ( | casacore::Float | clip = 10.0 , |
casacore::Float | sigma = -1.0 |
||
) |
casacore::ImageExpr<casacore::Float> casa::ImagePolarimetry::sigmaFracTotPol | ( | casacore::Float | clip = 10.0 , |
casacore::Float | sigma = -1.0 |
||
) |
casacore::Float casa::ImagePolarimetry::sigmaLinPolInt | ( | casacore::Float | clip = 10.0 , |
casacore::Float | sigma = -1.0 |
||
) |
Get the linearly polarized intensity image and its standard deviation.
If wish to debias the image, you can either provide sigma
(the standard deviation of the termal noise) or if sigma
is non-positive, it will be worked out for you with a clipped mean algorithm.
casacore::ImageExpr<casacore::Float> casa::ImagePolarimetry::sigmaLinPolPosAng | ( | casacore::Bool | radians, |
casacore::Float | clip = 10.0 , |
||
casacore::Float | sigma = -1.0 |
||
) |
casacore::Float casa::ImagePolarimetry::sigmaStokes | ( | ImagePolarimetry::StokesTypes | index, |
casacore::Float | clip = 10.0 |
||
) |
casacore::Float casa::ImagePolarimetry::sigmaStokesI | ( | casacore::Float | clip = 10.0 | ) |
casacore::Float casa::ImagePolarimetry::sigmaStokesQ | ( | casacore::Float | clip = 10.0 | ) |
casacore::Float casa::ImagePolarimetry::sigmaStokesU | ( | casacore::Float | clip = 10.0 | ) |
casacore::Float casa::ImagePolarimetry::sigmaStokesV | ( | casacore::Float | clip = 10.0 | ) |
casacore::Float casa::ImagePolarimetry::sigmaTotPolInt | ( | casacore::Float | clip = 10.0 , |
casacore::Float | sigma = -1.0 |
||
) |
casacore::IPosition casa::ImagePolarimetry::singleStokesShape | ( | casacore::CoordinateSystem & | cSys, |
casacore::Stokes::StokesTypes | type | ||
) | const |
Get the shape and casacore::CoordinateSystem of an image for a single Stokes pixel.
Thus, if the construction image shape was [10,10,4,20] where axis 2 (shape 4) is the casacore::Stokes axis, this function would return [10,10,1,20] Specify the type of casacore::Stokes pixel you want.
casacore::ImageExpr<casacore::Float> casa::ImagePolarimetry::stokes | ( | ImagePolarimetry::StokesTypes | index | ) | const |
Get the specified casacore::Stokes image and the standard deviation of the image.
This is worked out by first clipping outliers from the mean at the specified level.
casacore::ImageExpr<casacore::Float> casa::ImagePolarimetry::stokesI | ( | ) | const |
Get the Stokes I image and the standard deviation of the I image.
This is worked out by first clipping outliers from the mean at the specified level.
casacore::ImageExpr<casacore::Float> casa::ImagePolarimetry::stokesQ | ( | ) | const |
Get the casacore::Stokes Q image and the standard deviation of the Q image.
This is worked out by first clipping outliers from the mean at the specified level.
casacore::ImageExpr<casacore::Float> casa::ImagePolarimetry::stokesU | ( | ) | const |
Get the casacore::Stokes U image and the standard deviation of the U image.
This is worked out by first clipping outliers from the mean at the specified level.
casacore::ImageExpr<casacore::Float> casa::ImagePolarimetry::stokesV | ( | ) | const |
Get the casacore::Stokes V image and the standard deviation of the V image.
This is worked out by first clipping outliers from the mean at the specified level.
void casa::ImagePolarimetry::summary | ( | casacore::LogIO & | os | ) | const |
Summary.
Just invokes the casacore::ImageSummary list function to summarize the header of the construction image
casacore::ImageExpr<casacore::Float> casa::ImagePolarimetry::totPolInt | ( | casacore::Bool | debias, |
casacore::Float | clip = 10.0 , |
||
casacore::Float | sigma = -1.0 |
||
) |
Get the total polarized intensity (from whatever combination of Q, U, and V the construction image has) image and its error (standard deviation).
If wish to debias the image, you can either provide sigma
(the standard deviation of the thermal noise) or if sigma
is non-positive, it will be worked out for you with a clipped mean algorithm.
|
private |
Definition at line 403 of file ImagePolarimetry.h.
|
private |
const casacore::ImageInterface<casacore::Float>* _image;
Definition at line 393 of file ImagePolarimetry.h.
|
private |
Definition at line 391 of file ImagePolarimetry.h.
Referenced by coordinates(), imageInterface(), isMasked(), and shape().
|
private |
Definition at line 394 of file ImagePolarimetry.h.
|
private |
These blocks are always size 4, with IQUV in slots 0,1,2,3 If your image is IV only, they still use slots 0 and 3.
Definition at line 399 of file ImagePolarimetry.h.
|
private |
Definition at line 401 of file ImagePolarimetry.h.
|
staticprivate |
Definition at line 389 of file ImagePolarimetry.h.