Greg,
I apologize for so many questions!

Are those executables for Linux OS?
I use Windows 7 32-bit OS.


Message: 1
> Date: Mon, 20 Feb 2012 14:48:37 -0600
> From: "Tyukhova, Yulia" <[email protected]>
> To: [email protected]
> Subject: [HDRI] HDRI capture of LED
> Message-ID:
>        <CAJYAbgpa_tQtuxLAvgFeOQXzC0X8F25D6haBdt1uOqT=4nh...@mail.gmail.com
> >
> Content-Type: text/plain; charset="iso-8859-1"
>
> Everybody,
>
> Thank you for fast responses/tools and suggestions!
>
> Greg,
>
> Thank you for your suggestions and files!
> I am new to Radiance, and I assume that this is what I need to have
> installed on my computer in order to use suggested Perl scripts.
> If you can provide me with the link/info how to run it, that would be
> really helpful!
>
> Let me restate the question about the compression of the curve in
> Photosphere.
> 1. Do manufactures compress the response curve or maybe it is limited by
> camera/optics/sensor saturation itself on the upper end?
>
> 2. And I'm still curious, how CF is applied in Photosphere?
>
> I've been using ND filter t=0.0094 on the luminance meter, because
> otherwise it is impossible to measure such high luminances. I assume, you
> suggest to use it on the camera as well.
>
> I'm looking forward to analyze my images with the suggested
> hdrgen. Luckily, I've been taken them in both formats jpeg and raw.
> Greg, will you recommend to have regular calibration scene calibrated at
> the grey card instead of using brighter scene?
>
> Thank you,
> Yulia
>
> Hello Yulia,
>
> Seems your question has spawned quite a bit of interesting discussion...
>
> My main recommendation is to use camera RAW images for critical photometry,
> especially when there are saturated colors involved.  It is impossible to
> correct the color of JPEG images and undo what the camera maker has done,
> so you need to start from the sensor data.
>
> Photosphere does not accept camera RAW as input, but I have written a Perl
> script that uses dcraw with the command-line HDR image builder hdrgen to
> overcome this limitation.  It also requires the use of another third-party
> program, exiftool, which I have packaged together for you at:
>
>       http://www.anyhere.com/gward/pickup/raw2hdr.tgz
>
> Unfortunately, I don't have a good set of documentation to go with it.
>  Typing "raw2hdr" by itself shows the basic syntax:
>
>       Usage: raw2hdr [hdrgen opts][-h][-w][-C calib][-c cspace] -o
> output.hdr input1.raw ..
>
> If your images are taken on a tripod (aligned exposures), you can use the
> default settings:
>
>       raw2hdr -o output.hdr expos1.cr2 expos2.cr2 expos3.cr2 ...
>
> The hdrgen settings can be found in the included HTML man page, and so can
> the -h and -w option meanings in the included dcraw man page.  The -C
> option is to provide a linear factor to correct the overall exposure based
> on previous calibrations.  The -c option is to specify an output color
> space.  The default is "sRGB" which is actually linear CCIR-709 primaries.
>  The only other output color space I would recommend is AdobeRGB.  There is
> a CIE XYZ space supported by dcraw, but I have found it to be somewhat
> unreliable, and I don't know where the fault lies in this.
>
> Regarding Axel's mention of camera flare, this is less of an issue for
> sources that are brighter than the rest of the scene.  It mostly affects
> darker, surrounding regions.  The -f option will attempt to estimate the
> camera/lens PSF and remove it, but it cannot be relied upon to remove this
> source of error completely.  Your problem with the accuracy of the LED
> sources is due no doubt (as others have said) to limitations in your short
> exposures combined with the color issues inherent to JPEG processing.
>
> Other responses inline....
>
> > From: "Tyukhova, Yulia" <[email protected]>
> > Date: February 19, 2012 9:34:25 PM PST
> >
> > Hello everybody!
> > I?ll provide the summary of my research and have questions within the
> summary. I would appreciate any of your help!
> > My research investigates if HDRI technique can precisely capture
> luminances of small bright light sources (e.g. LED garage fixtures) with
> narrow light distributions.
> > I was able to figure out luminance values for a single LED, which can be
> compared to the ones from HDR images. But I have a couple of
> questions/concerns on HDRI technique and Photosphere.
> > At first, I?ve used ?regular? scene to retrieve response curve of the
> camera (large smooth gradients with very dark and bright areas, and had
> reflectance standards for the absolute calibration).
> > Camera: EOS T1i Rebel with 28-105mm lens, at 28mm
> > Calibrated at the grey reflectance sample 186.45 cd/m2
> > CF=0.957
> >
> > I?ve got the following RC for RGB:
> > red(r) = -6.434199e-03+ 4.518039e-01*r + 1.291426e+00*r^2 +
> 1.802896e+00*r^3;
> > green(g) = -5.804720e-03+ 4.175837e-01*g + 1.176582e+00*g^2 +
> 1.721643e+00*g^3;
> > blue(b) = -4.376831e-03+ 3.784418e-01*b + 1.075695e+00*b^2 +
> 1.658471e+00*b^3
> > If I look at the histogram of the scene, maximum luminance within the
> scene is 60,291 cd/m2.
> > Then I use this RC to analyze HDRI of a captured LED. The value is
> 230,000 cd/m2 for a single LED, which is low (it?s has to be around 7*106
> cd/m2). So, it underestimates the luminance.
> > It seems like calibration point is critical here. I?ve decided to try to
> capture a different scene for deriving RC with a wider range. It would make
> sense that camera has to see higher luminance values in order to accurately
> measure them later. The dynamic range has to cover measured values.
> > 1.    How does Photosphere deals/approximates/calculates the upper end of
> the curve? I assume it gives more weight to mid tone values? But what
> happens with high luminance values?
> Photosphere (and hdrgen) use all the brightest pixels from the shortest
> exposure and all the darkest pixels from the longest exposure.  Middle
> exposures have their brightest and darkest pixels downgraded.
> > So, the new brighter scene was picked with the direct sun! But in order
> to avoid the damage of the camera?s sensor, measurements were taken before
> the sunset.
> > In the new brighter captured scene without the calibration all values for
> reflectance standards were overestimated, while the value for the sun
> underestimated. Then I decided to calibrate my scene at the sun!
> > But when I apply absolute calibration, it simply multiplies CF to all
> values.
> > 2.     I assumed when CF is applied, it does not equally change all
> values, but does it proportionally to RC (since it is not linear).  Why
> does it do it equally for the whole range?
> > Lsun=80*106 cd/m2. And of course CF is very big 391.
> > New RC:
> > red(r) = 3.219064e+00+ -2.655078e+01*r + 9.351069e+02*r^2 +
> -2.115052e+03*r^3+1.594538e+03*r^4;
> > green(g) = 2.094164e+00+ -1.468109e+00*g + 7.306838e+02*g^2 +
> -1.720743e+03*g^3+1.380693e+03*g^4;
> > blue(b) = 1.049078e+00+ 1.591820e+01*b + 5.848958e+02*b^2 +
> -1.461635e+03*b^3+1.251033e+03*b^4
> > But then something interesting happened. When I analyze LED, it gives a
> value of 79*106 cd/m2. So, it jumps to this upper limit calibrated with the
> sun previously.
> > (I had similar results for EOS 7D with the lens 16-35mm, at 16mm)
> >
>
> I don't think your shortest exposure properly captured the LED, and maybe
> didn't capture the sun, either.
> > 3.     Does photosphere compress the response curve, so at the upper end
> all values above certain threshold will have the same number?
>
> Photosphere does not compress the curve.
> > 4.     Any additional suggestions on properly obtaining and calibrating
> HDRI for this purpose?
>
> I would only reiterate others' suggestion to use a neutral density filter,
> and using raw2hdr rather than Photosphere.
>
> > --
> > Thank you,
> > Yulia Tyukhova
>
> Best,
> -Greg
>
> --
> Thank you,
> *Yulia Tyukhova*
> *
> *
> Fulbright Scholar, "Intern LC"
> Architectural Engineering Graduate Student, UNL-Omaha, NE, USA
> B.E. and M.E. in Lighting Engineering (MPEI), Moscow, Russia
> [email protected]
> [email protected]
> +1 (402) 996 0910
> PKI 247
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> ------------------------------
>
> Message: 2
> Date: Mon, 20 Feb 2012 13:14:15 -0800
> From: "Gregory J. Ward" <[email protected]>
> To: High Dynamic Range Imaging <[email protected]>
> Subject: Re: [HDRI] HDRI capture of LED
> Message-ID: <[email protected]>
> Content-Type: text/plain; charset="us-ascii"
>
> Responses inline...
>
> > From: "Tyukhova, Yulia" <[email protected]>
> > Date: February 20, 2012 12:48:37 PM PST
> >
> > Everybody,
> >
> > Thank you for fast responses/tools and suggestions!
> >
> > Greg,
> >
> > Thank you for your suggestions and files!
> > I am new to Radiance, and I assume that this is what I need to have
> installed on my computer in order to use suggested Perl scripts.
> > If you can provide me with the link/info how to run it, that would be
> really helpful!
>
> Actually, you don't need to have Radiance installed.  You just need to
> move the executables (non-HTML files) from the unpacked directory to
> /usr/bin or /usr/local/bin or some other directory in your shell's PATH
> variable.  These are command-line tools that must be run from the Terminal
> application under /Applications/Utilities.  I.e., start Terminal and copy
> the files from your Downloads folder with:
>
>        cd Downloads
>        tar xzf raw2hdr.tgz
>        cd raw2hdr
>        cp raw2hdr dcraw exiftool /usr/bin
>        cd
>        raw2hdr
>
>


> This should give you the usage message I wrote you earlier if it all goes
> well.  Some basic commands and pointers for Unix are available many places
> online.  Googling "basic unix tutorial" gave this page at the head of the
> list:
>
>        http://www.ee.surrey.ac.uk/Teaching/Unix/
>
> > Let me restate the question about the compression of the curve in
> Photosphere.
> > 1. Do manufactures compress the response curve or maybe it is limited by
> camera/optics/sensor saturation itself on the upper end?
>
> Some camera makers do compress the top end of the response curve, and do
> funny things at the bottom as well.  Photosphere attempts to discover the
> tone curve and correct for these manipulations, but it isn't perfect and if
> the camera is changing the tone curve dynamically, it's pretty hopeless.
>  There are settings you can use on a DSLR to disable such manipulations,
> but using RAW files bypasses the problems entirely because the data is
> linear.
>
> > 2. And I'm still curious, how CF is applied in Photosphere?
>
> A calibration factor is applied equally to all coefficients in the
> polynomial, which is exactly the same as applying a linear scale factor
> after the HDR merge operation.
>
> > I've been using ND filter t=0.0094 on the luminance meter, because
> otherwise it is impossible to measure such high luminances. I assume, you
> suggest to use it on the camera as well.
>
> Whatever gives you a short exposure that is past the integration time of
> your source (1/60th second is acceptable) and not saturated is OK.
>  Specifically, all values in the short exposure's histogram should be be
> below 245.
>
> > I'm looking forward to analyze my images with the suggested hdrgen.
> Luckily, I've been taken them in both formats jpeg and raw.
> > Greg, will you recommend to have regular calibration scene calibrated at
> the grey card instead of using brighter scene?
>
> The best scene for calibration is a white card in a scene with no bright
> sources directed at the camera.  The calibration should hold in other
> scenes where lens flare is not problematic.
>
> > Thank you,
> > Yulia
>
> Certainly,
> -Greg
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> End of HDRI Digest, Vol 46, Issue 7
> ***********************************
>



-- 
Thank you,
*Yulia Tyukhova*
*
*
Fulbright Scholar, "Intern LC"
Architectural Engineering Graduate Student, UNL-Omaha, NE, USA
B.E. and M.E. in Lighting Engineering (MPEI), Moscow, Russia
[email protected]
[email protected]
+1 (402) 996 0910
PKI 247
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