Revision as of 17:12, 13 October 2018

1 Hint:

Create a variable containing your Betas IP for easy access.

export BETA=192.168.1.101

2 Preparations

Install on your AXIOM Beta:

pacman -S python-numpy

Install the following packages on your PC:

dcraw octave

For Ubuntu this would look like:

sudo apt-get install dcraw octave

Download and compile raw2dng on your PC: https://github.com/apertus-open-source-cinema/misc-tools-utilities/tree/master/raw2dng

2.1 Step 1: Check range of the input signal

On the Beta set gain to x1 by running:

./set_gain.sh 1

Download this Octave file to your PC into your current work directory:

wget https://raw.githubusercontent.com/apertus-open-source-cinema/misc-tools-utilities/master/darkframes/read_raw.m

Capture an overexposed image with the Beta and check the levels:

ssh root@$BETA "./cmv_snap3 -2 -b -r -e 100ms" > snap.raw12 

./raw2dng snap.raw12 --totally-raw

octave

   octave:1> a = read_raw('snap.DNG')

   octave:2> prctile(a(:), [0.1 1 50 99 99.9])

If everything worked you will get a wall of numbers now. TODO: We should extract the essential pieces of information here... (min/max maybe)?

Lower numbers should be around 50...300 (certainly not zero). Higher numbers should be around 4000, but not 4095.

Repeat for gains 2, 3, 4.

Put this in startup script (ie: kick_manual.sh) :

./set_gain.sh 1

2.2 Step 2: RCN calibration

RCN stands for Row Coloumn Noise correction meaning we filter out the fixed pattern noise.

Make sure you have these scripts already in your Betas /root/ directly: https://github.com/apertus-open-source-cinema/beta-software/tree/master/software/scripts

Clear the old RCN values:

ssh root@$BETA "./rcn_clear.py"

Now you need to make sure that your Beta is not capturing any light (really not a single photon should hit the sensor :) ):

close the lens aperture as far as possible
attach lens cap
put black lens bag over Beta
turn off all lights in the room - do this at night or in a completely dark room

Take 64 dark frames at 10ms, gain x1 with the following script executed on your PC (1.2 GB needed):

ssh root@$BETA " ./set_gain.sh 1" 

ssh root@$BETA ". ./cmv.func; fil_reg 15 0" # disable HDMI stream 

for i in `seq 1 64`; do 

  ssh root@$BETA "./cmv_snap3 -2 -b -r -e 10ms" > dark-x1-10ms-$i.raw12  

done  

ssh root@$BETA ". ./cmv.func; fil_reg 15 0x01000100"  # enable HDMI stream

Compute a temporary dark frame for RCN calibration:

raw2dng --swap-lines --no-blackcol --calc-darkframe dark-x1-10ms-*.raw12

This should process quite quickly and output something like the following at the end:

Averaged 64 frames exposed from 12.00 to 12.00 ms. 

Could not compute dark current. 

Please use different exposures, e.g. from 1 to 50 ms. 

Dark offset : 0.00 

Writing darkframe-x1.pgm... 

Done.

Rename and upload darkframe to your Beta:

mv darkframe-x1.pgm darkframe-rcn.pgm 

scp darkframe-rcn.pgm root@$BETA:/root/

Set the RCN values:

ssh root@$BETA "./rcn_darkframe.py darkframe-rcn.pgm"

Put this in startup script (ie : kick_manual.sh) :

./rcn_darkframe.py darkframe-rcn.pgm

If you get an error report like this:

Traceback (most recent call last): 

 File "rcn_darkframe.py", line 17, in <module> 

   import png 

ImportError: No module named 'png'

Make sure the Beta is connected to the Internet via Ethernet and run:

pip install pypng

and then run the python script again

2.2.1 Validation

2.2.1.1 Method 1:

Put a lens cap on the camera and check the image on a HDMI monitor.

In the camera set the matrix gains to:

./mat4_conf.sh  20 0 0 0  0 10 10 0  0 10 10 0  0 0 0 10  0 0 0 0

run:

./rcn_clear.py

The static noise profile should be visible.

run:

./rcn_darkframe.py darkframe-rcn.pgm

The static noise profile should be gone. You will still see dynamic row noise (horizontal lines flickering) - thats expected.

2.2.1.2 Method 2:

This method is now entirely automated with running one script inside the camera: https://github.com/apertus-open-source-cinema/beta-software/blob/master/software/scripts/rcn_validation.sh

Capture one darkframe without compensations:

ssh root@$BETA "./rcn_clear.py" 

ssh root@$BETA "./cmv_snap3 -2 -b -r -e 10ms" > dark-check-1.raw12

Capture one darkframe with compensations:

ssh root@$BETA "./rcn_darkframe.py darkframe-rcn.pgm" 

ssh root@$BETA "./cmv_snap3 -2 -b -r -e 10ms" > dark-check-2.raw12

Then use raw2dng to analyze the differences:

raw2dng --no-darkframe --check-darkframe dark-check-1.raw12 

raw2dng --no-darkframe --check-darkframe dark-check-2.raw12

With the compensated snapshot the column noise should disappear, and only row noise left should be dynamic (not static). Visual inspection: the dark frame should have only horizontal lines, not vertical ones.

Sample output:

Average     : 127.36               # about 128, OK 

Pixel noise : 5.44                 # this one is a bit high because we only corrected row and column offsets (it's OK) 

Row noise   : 2.30 (42.2%)         # this one should be only dynamic row noise - see Method 3 below. 

Col noise   : 0.20 (3.8%)          # this one is very small, that's what we need to check here

2.2.1.3 Method 3:

Capture 2 frames:

ssh root@$BETA "./cmv_snap3 -2 -b -r -e 10ms" > dark-check-1.raw12  

ssh root@$BETA "./cmv_snap3 -2 -b -r -e 10ms" > dark-check-2.raw12

Convert the two darkframes with raw2dng:

raw2dng dark-check-*

Make sure you have the required octave function file in place:

wget https://raw.githubusercontent.com/apertus-open-source-cinema/misc-tools-utilities/master/darkframes/read_raw.m

Also you need to install the octave "signal" and "control" packages from: http://octave.sourceforge.net/packages.php then inside octave run to install:

pkg install package_name

To check whether the entire row noise is dynamic, load the two raw images in octave and check the autocorrelation between the two row noise samples:

pkg load signal 

a = read_raw('dark-check-1.DNG'); 

b = read_raw('dark-check-2.DNG'); 

ra = mean(a'); ra = ra - mean(ra); 

rb = mean(b'); rb = rb - mean(rb); 

xcov(ra, rb, 0, 'coeff')

Result should be very small (about 0.1 or lower). When running this check on two uncalibrated dark frames, you will get around 0.8 - 0.9.

2.3 Step 3: Dark frame calibration

Make sure the RCN calibration from previous steps is in place before continueing here.

Take 1600 dark frames at various exposure times and gains. This will require around 30GB of space on your PC.

for i in 1 2 3 4; do
  for e in `seq 1 100`; do
    for g in 1 2 3 4; do
      ssh root@$BETA "./set_gain.sh $g"
      ssh root@$BETA "./cmv_snap3 -2 -b -r -e ${e}ms" > dark-x${g}-${e}ms-$i.raw12
    done
  done
done

Compute dark frames for each gain:

raw2dng --calc-dcnuframe dark-x1-*.raw12
raw2dng --calc-dcnuframe dark-x2-*.raw12
raw2dng --calc-dcnuframe dark-x3-*.raw12
raw2dng --calc-dcnuframe dark-x4-*.raw12

This produces the following files:

darkframe-x1.pgm, dcnuframe-x1.pgm, darkframe-x2.pgm, dcnuframe-x2.pgm, darkframe-x3.pgm, dcnuframe-x3.pgm, darkframe-x4.pgm, dcnuframe-x4.pgm

Store these files in a save place as they will be used in post-processing. Place them in the directory where you capture raw12 files or experimental raw HDMI recordings, so raw2dng will use them.

2.3.1 Validation

Capture a few new raw12 darkframes with rcn enabled and PGMs in place for raw2dng.

raw2dng --check-darkframe dark*.raw12 > dark-check.log

If the calibration worked you should get lower noise values as in step 2.

average value: close to 128

pixel noise: about 3 or 4 (may increase at longer exposure times)

row noise and column noise should look similar to this:

Pixel noise : 3               
Row noise   : 1.70     
Col noise   : 0.15

2.4 Step 4: Color profiling

Set gain x1.

ssh root@$BETA "./set_gain.sh 1"

Take a picture of the IT8 chart, correctly exposed.

Edit the coordinates and the raw file name in calib_argyll.sh.

ssh root@$BETA "./cmv_snap3 -2 -b -r -e 10ms" > it8chart.raw12
./calib_argyll.sh IT8

Save the following files:

ICC profile (*.icc)
OCIO configuration (copy/paste from terminal) + LUT file (*.spi1d)

2.4.1 Validation

Render the IT8 chart in Blender, using the OCIO configuration.

Same with the ICC profile (Adobe? RawTherapee? What apps support ICC?)

(todo: detailed steps)

2.5 Step 5: HDMI dark frames

For experimental 4k raw recording (https://www.apertus.org/axiom-beta-uhd-raw-mode-explained-article-may-2016) step 3 calibration is not required (step 2 should be in place though). Instead darkframes are collected from HDMI recordings.

Record a 1-minute clip with lens cap on.

Average odd and even frames.

(todo: polish and upload the averaging script)

(todo: check if the HDMI dark frames can be computed from regular dark frames)

Results: darkframe-hdmi-A.ppm and darkframe-hdmi-B.ppm.

2.6 Step 6: HDMI filters for raw recovery

This calibration is for to the recorder, not for the camera. It's for recovering the original raw data from the HDMI, so it has nothing to do with sensor profiling and such.

Record some scene with high detail AND rich colors.

Take a raw12 snapshot in the middle of recording. The HDMI stream will pause for a few seconds.

Upload two frames from the paused clip, together with the raw12 file. This calibration will be hardcoded in hdmi4k.

The two frames must be in the native format of your video recorder (not DNG). You should be able to cut the video with ffmpeg -vcodec copy.

2.7 TODO

batch script to copy all the utilities for the workflow
implement this: https://wiki.apertus.org/index.php/Calibration_files
automate HDMI calibration
remind Herbert to fix the line swapping bug

Difference between revisions of "Factory Calibration"