Contents
2014-01-22 Meeting minutes
Hi everyone,
Here is a short summary of what I heard today for how we should start
with the pnCCD.
For pnCCD algorithms:
common-mode, pedestals, hot-pixels, quadrant rotations, hit-finders,
support in mikhail's calibManager
For pnCCD online displays: (using matplotlib for now)
shot by shot raw data
shot by shot calibrated data
projections of the above
region-of-interest
strip-charts of interesting quantities
(also display calibration values like noise-map,pedestal-map)
After this we will work on the acqiris as well (acqiris
constant-fraction algos already exist in psana).
Attached below is a 12 line python program that plots a real pnCCD
image and an x-projection (amoc0113 also has pnccd data we can look
at). You can run it on a psana node by saving it to pnccd.py and
doing "sit_setup" and then "ipython pnccd.py". This sort of code
should work online too (although we may have to change matplotlib
settings) as well as with calibrated images.
Display group (dan, mikhail, me) meets Thursday at 10:30. Analysis
group (sebastian, ankush(?), phil, mikhail, me) meets Friday at 1.
See you then...
chris
Script form Chris
Use interactive psana framework ~cpo/ipsana/shm.py
:
from psana import * events = DataSource('shmem=1_1_XCS.0').events() src = Source('DetInfo(XcsBeamline.1:Tm6740.5)') import matplotlib.pyplot as plt plt.ion() fig = plt.figure('pulnix') ax = fig.add_axes([0.1, 0.1, 0.8, 0.8]) # x0, y0, h, w for i in range(100): evt = events.next() frame = evt.get(Camera.FrameV1, src) ax.cla() ax.imshow(frame.data16()) fig.canvas.draw()
Walking and talking about unlimited pipeline (processing)
CASS Heritage
Online monitor
Data for tests
On 2014-01-27 Sebastian Carron kindly provide us with data files for pnCCD experiment amoa1214:
- Dark Run: 169, rear sensors gain 1/64, front 1/1, Imaging mode exp=amoa1214:run=169
- Run With Hits: 170 Low hit rate though, so you will have to use a hit finder of sorts exp=amoa1214:run=170
Calibration of pnCCD
New modules for "old-style" calibration:
- pdscalibdata/include/PnccdBaseV1.h - baseclass for pnCCD parameters, defines Segs, Rows, Cols, Size
- pdscalibdata/include/PnccdPedestalsV1.h - loads pedestals from file, returns ndarray of pedestals
- pdscalibdata/include/PnccdCommonModeV1.h - the same for common mode
- pdscalibdata/include/PnccdPixelGainV1.h - the same for pixel gain
- pdscalibdata/include/PnccdPixelRmsV1.h - the same for pixel rms
- pdscalibdata/include/PnccdPixelStatusV1.h - the same for pixel status
- PSCalib::PnccdCalibPars - wrapper for all pnCCD types
Detector-dependent interface
Example can be found in PSCalib/test/ex_calib_file_finder.cpp:
// Assume that file is located in /reg/d/psdm/AMO/amotut13/calib/PNCCD::CalibV1/Camp.0:pnCCD.1/pedestals/1-end.data #include "PSCalib/PnccdCalibPars.h" const std::string calib_dir = "/reg/d/psdm/AMO/amotut13/calib"; const std::string group = "PNCCD::CalibV1"; // or std::string() const std::string source = "Camp.0:pnCCD.1"; unsigned long runnum = 10; unsigned print_bits = 255; PSCalib::PnccdCalibPars *calibpars = new PSCalib::PnccdCalibPars(calib_dir, group, source, runnum, print_bits); calibpars->printCalibPars(); calibpars->printCalibParsStatus(); calibpars->printInputPars(); ndarray<CalibPars::pedestals_t, 3> peds = calibpars -> pedestals_ndarr(); ndarray<CalibPars::common_mode_t, 1> cmod = calibpars -> common_mode_ndarr(); ndarray<CalibPars::pixel_status_t, 3> stat = calibpars -> pixel_status_ndarr(); ndarray<CalibPars::pixel_gain_t, 3> gain = calibpars -> pixel_gain_ndarr(); ndarray<CalibPars::pixel_rms_t, 3> gain = calibpars -> pixel_gain_ndarr(); // OR: CalibPars::pedestals_t* p_peds = calibpars -> pedestals(); CalibPars::common_mode_t* p_cmod = calibpars -> common_mode(); CalibPars::pixel_status_t* p_stat = calibpars -> pixel_status(); CalibPars::pixel_gain_t* p_gain = calibpars -> pixel_gain(); CalibPars::pixel_rms_t* p_gain = calibpars -> pixel_gain(); const size_t ndim = ndim(); const size_t size = size(); const unsigned* shape = shape(); etc...
Pros
- Simple format for calibration files - just a text file with pre-defined number of values for each type:
973.941639 881.189675 1050.211 773.263749 899.241302 981.805836 1150.72615 993.084175 1121.15488 1029.76319 1220.14927 903.278339 1097.49944 1066.94949 1263.71044 1053.53872 1194.35915 935.320988 1317 ...
Cons
- Too simple calibration file format, does not allow any metadata or comments.
- Detector-dependent objects and parameters "knows" about parameters' array type and shape:
- PSCalib::PnccdCalibPars which depends on PnccdPedestalsV1, PnccdCommonModeV1, ..., PnccdBaseV1
pdscalibdata::PnccdPedestalsV1::pars_t = float
pdscalibdata::PnccdCommonModeV1::pars_t = uint16_t
pdscalibdata::PnccdPixelStatusV1::pars_t = uint16_t
pdscalibdata::PnccdPixelGainV1::pars_t = float
- const std::string groupName = "PNCCD::CalibV1"; - do we really need it ?
Detector-independent interface
- Interface is declared in the abstract base class PSCalib::CalibPars
- Access to all detector-dependent classes is hidden in the static factory class PSCalib::CalibParsStore
Factory is implemented for pnCCD only. CSPAD and CSPAD2x2 will be added soon.
#include "PSCalib/CalibPars.h" #include "PSCalib/CalibParsStore.h" // Instatiation //Here we assume that code is working inside psana module where evt and env variables are defined through input parameters of call-back methods. //Code below instateates calibpars object using factory static method PSCalib::CalibParsStore::Create: std::string calib_dir = env.calibDir(); // or "/reg/d/psdm/<INS>/<experiment>/calib" std::string group = std::string(); // or something like "PNCCD::CalibV1"; const std::string source = "Camp.0:pnCCD.1"; const std::string key = ""; // key for raw data Pds::Src src; env.get(source, key, &src); PSCalib::CalibPars* calibpars = PSCalib::CalibParsStore::Create(calib_dir, group, src, PSCalib::getRunNumber(evt)); // Access methods calibpars->printCalibPars(); const PSCalib::CalibPars::pedestals_t* peds_data = calibpars->pedestals(); const PSCalib::CalibPars::pixel_gain_t* gain_data = calibpars->pixel_gain(); const PSCalib::CalibPars::pixel_rms_t* rms_data = calibpars->pixel_rms(); const PSCalib::CalibPars::pixel_status_t* stat_data = calibpars->pixel_status(); const PSCalib::CalibPars::common_mode_t* cmod_data = calibpars->common_mode();
New approach to calibration files with header
In order to get rid of detector dependent types of calibration parameters we need to add metadata in the calibration file. All metadata can be listed in the header of the calibration files, for example, using keyward mapping (dictionary):
# RULES: # Lines starting with # in the beginning of the file are considered as comments or pseudo-comments for metadata # Lines without # with space-separated values are used for input of parameters # Empty lines are ignored # Optional fields: # TITLE: This is a file with pedestals # DATE_TIME: 2014-01-30 10:21:23 # AUTHOR: someone # EXPERIMENT: amotut13 # DETECTOR: Camp.0:pnCCD.1 # CALIB_TYPE: pedestals # Mandatory fields to define the ndarray<TYPE,NDIMS> and its shape as unsigned shape[NDIMS] = {DIM1,DIM2,DIM3} # TYPE: float # NDIMS: 3 # DIM1: 4 # DIM2: 255 # DIM3: 255 973.941639 881.189675 1050.211 773.263749 899.241302 981.805836 1150.72615 993.084175 1121.15488 1029.76319 1220.14927 903.278339 1097.49944 1066.94949 1263.71044 1053.53872 1194.35915 935.320988 1317 ...
psana modules for pnCCD
New module ImgAlgos.PnccdNDArrProducer
- Get from the event store
Psana::PNCCD::FramesV1
, - Put in the event store
ndarray<T,3>, where shape=[4][512][512], T=uint16_t, int, float, double, int16_t
Performance: ~13 ms/event
Modified module ImgAlgos.PnccdImageProducer
- Get from the event store
Psana::PNCCD::FullFrameV1
orndarray<T,3>
forsource
andkey
parameters - Put in the event store
ndarray<T,2>, where shape=[1024+gap][1024], T= input type
Performance: ~30 ms/event (copy involves inverse iteration for 180 degree rotation of two bottom frames)
Old sequence of image averaging
ImgAlgos.PnccdImageProducer - get Psana::PNCCD::FullFrameV1, put ndarray<uint16_t, 2>
ImgAlgos.NDArrAverage - averages ndarray<T, 2>, save in file
New sequence of image averaging
For demonstration only! Just in order to confirm that we produce the same image from different objects. In real case image needs to be produced at final stage.
ImgAlgos.PnccdNDArrProducer - get Psana::PNCCD::FramesV1
, put ndarray<T, 3>
ImgAlgos.PnccdImageProducer - get ndarray<T,3>, put ndarray<T, 2>
ImgAlgos.NDArrAverage - averages ndarray<T, 2>, save in file
"Natural order" for common mode correction in pnCCD ndarray
pnCCD image has intensity "strips" in both dimensions;
[4][512][512] array for single event and averaged over 1000 events:
At large number of events common mode should be averaged out. For 1000 events horizontal intensity "stripes" have gone.
This proves that common mode should be evaluated for horizontal stripes.
Data corrections in module ImgAlgos.NDArrCalib
List of parameters in configuration file
[ImgAlgos.NDArrCalib] source = DetInfo(Camp.0:pnCCD.0) key_in = pnccd-ndarr key_out = calibrated do_peds = yes do_cmod = no do_stat = no do_mask = no do_bkgd = no do_gain = no do_nrms = no do_thre = yes fname_bkgd = fname_mask = masked_value = 0 threshold_nrms = 0 threshold = 100.0 below_thre_value = 50 bkgd_ind_min = 0 bkgd_ind_max = 1000 bkgd_ind_inc = 2 print_bits = 11
Pedestals subtraction
Calibration type: pedestals
Threshold
Apply common threshold = 100 ADU:
peak in spectrum at 0 corresponds settings for gap
peak in spectrum at 50 corresponds settings for under threshold pixels
Gain
Calibration type: pixel_gain
Apply common gain factor = 0.5:
Pixel status mask
Calibration type: pixel_status (0-good, 1,2,4,...-bad)
Set bad pixels (1) in the half of frame[1]:
2014-02-06 pnccd with common mode
Dark run: exp=amoa1214:run=7, all plots are shown for Camp.0:pnCCD.0
event 5
Pedestals are generated for ndarray using the same dark run
Raw data
Pedestals subtracted
Pedestals and common mode subtracted
Using intensity distribution for pedestals set
/reg/d/psdm/AMO/amoa1214/calib/PNCCD::CalibV1/Camp.0:pnCCD.0/common_mode/1-end.data
1 300 50
Average over 128 pixels
Common mode subtraction improves the width of intensity distribution.
Get latest version of packages for psana and calibman
ssh -Y psana cd <your-favorite-directory> newrel ana-current <release-directory> cd <release-directory> sit_setup addpkg ImgAlgos HEAD; addpkg pdscalibdata HEAD; addpkg PSCalib HEAD; addpkg CalibManager HEAD; scons;