Does anyone know the statistics of cub_200? I need mean and std of each channel and I want to make a shortcut and not calculate it myself :D
I got the mean from a repo which is (0.407, 0.457, 0.485) but it didn't have the std.
Related
Consider me a newbie at programming. I tried to search for an answer to this question before posting but no luck.
I am using CvAvgSdv function to calculate the Std Deviation and the Mean of the ROI of an image. For reference that is:
cvAvgSdv(LeftROI, LeftMean, LeftStdDev);
LeftMean & LeftStdDev are the output arrays in the form of *CvScalar but how do I display them/access the output value? I personally only need the Standard Deviation value as I am calculating the pixel variance in an image. So squaring the Standard Deviation should give me this.
Regards,
Sheraz
I write application where I must process digital signal - array of double. I must the signal decimate, filter etc.. I found a project gnuradio where are functions for this problem. But I can't figure how to use them correctly.
I need signal decimate (for example from 250Hz to 200Hz). The function should be similar to resample function in Matlab. I found, the classes for it are:
rational_resampler_base_fff Class source
fir_filter_fff Class source
...
Unfortunately I can't figure how to use them.
gnuradio and shared library I have installed
Thanks for any advice
EDIT to #jcoppens
Thank you very much for you help.
But I must process signal in my code. I find classes in gnuradio which can solve my problem, but I need help how set them.
Functions which I must set are:
low_pass(doub gain, doub sampling_freq, doub cutoff_freq, doub transition_width, window, beta)
where:
use "window method" to design a low-pass FIR filter
gain: overall gain of filter (typically 1.0)
sampling_freq: sampling freq (Hz)
cutoff_freq: center of transition band (Hz)
transition_width: width of transition band (Hz).
The normalized width of the transition band is what sets the number of taps required. Narrow –> more taps
window_type: What kind of window to use. Determines maximum attenuation and passband ripple.
beta: parameter for Kaiser window
I know, I must use window = KAISER and beta = 5, but for the rest I'm not sure.
The func which I use are: low_pass and pfb_arb_resampler_fff::filter
UPDATE:
I solved the resampling using libsamplerate
I need signal decimate (for example from 250Hz to 200Hz)
WARNING: I expressed the original introductory paragraph incorrectly - my apologies.
As 250 Hz is not related directly to 200 Hz, you have to do some tricks to convert 250Hz into 200Hz. Inserting 4 interpolated samples in between the 250Hz samples, lowers the frequency to 50Hz. Then you can raise the frequency to 200Hz again by decimating by a factor 4.
For this you need the "Rational Resampler", where you can define the subsample and decimate factors. Something like this:
This means you would have to do something similar if you use the library. Maybe it's even simpler to do it without the library. Interpolate linearly between the 250 Hz samples (i.e. insert 4 extra samples between each), then decimate by selecting each 4th sample.
Note: There is a Signal Processing forum on stackexchange - maybe this question might fall in that category...
More information: If you only have to resample your input data, and you do not need the actual gnuradio program, then have a look at this document:
https://ccrma.stanford.edu/~jos/resample/resample.pdf
There are several links to other documents, and a link to libresample, libresample4, and others, which may be of use to you. Another, very interesting, page is:
http://www.dspguru.com/dsp/faqs/multirate/resampling
Finally, from the same source as the pdf above, check their snd program. It may solve your problem without writing any software. It can load floating point samples, resample, and save again:
http://ccrma.stanford.edu/planetccrma/software/soundapps.html#SECTION00062100000000000000
EDIT: And yet another solution - maybe the simplest of all: Use Matlab (or the free Octave version):
pkg load signal
t = linspace(0, 10*pi, 50); % Generate a timeline - 5 cycles
s = sin(t); % and the sines -> 250 Hz
tr = resample(s, 5, 4); % Convert to 200 Hz
plot(t, s, 'r') % Plot 250 Hz in red
hold on
plot(t, tr(1:50)) % and resampled in blue
Will give you:
I have Problem understanding all Parameter of backgroundsubtractormog2.
I looked in the code (located in bfgf_gaussmix2.cpp), but don't see the connection to the mentioned paper. For exmaple is Tb = varThreshold, but what is the name of Tb in the paper?
I am especially interested in the fat marked parameter.
Let's start with the easy parameter [my remarks]:
int nmixtures
Maximum allowed number of mixture components. Actual number is determined dynamically per pixel.
[set 0 for GMG]
uchar nShadowDetection
The value for marking shadow pixels in the output foreground mask. Default value is 127.
float fTau
Shadow threshold. The shadow is detected if the pixel is a darker version of the background. Tau is a threshold defining how much darker the shadow can be. Tau= 0.5 means that if a pixel is more than twice darker then it is not shadow.
Now to the ones i don't understand:
float backgroundRatio
Threshold defining whether the component is significant enough to be included into the background model ( corresponds to TB=1-cf from the paper??which paper??). cf=0.1 => TB=0.9 is default. For alpha=0.001, it means that the mode should exist for approximately 105 frames before it is considered foreground.
float varThresholdGen
Threshold for the squared Mahalanobis distance that helps decide when a sample is close to the existing components (corresponds to Tg). If it is not close to any component, a new component is generated. 3 sigma => Tg=3*3=9 is default. A smaller Tg value generates more components. A higher Tg value may result in a small number of components but they can grow too large. [i don't understand a word of this]
In the Constructor the variable varThreshold is used. Is it the same as varThresholdGen?
Threshold on the squared Mahalanobis distance to decide whether it is well described by the background model (see Cthr??). This parameter does not affect the background update. A typical value could be 4 sigma, that is, varThreshold=4*4=16; (see Tb??).
float fVarInit
Initial variance for the newly generated components. It affects the speed of adaptation. The parameter value is based on your estimate of the typical standard deviation from the images. OpenCV uses 15 as a reasonable value.
float fVarMin
Parameter used to further control the variance.
float fVarMax
Parameter used to further control the variance.
float fCT
Complexity reduction parameter. This parameter defines the number of samples needed to accept to prove the component exists. CT=0.05 is a default value for all the samples. By setting CT=0 you get an algorithm very similar to the standard Stauffer&Grimson algorithm.
Someone asked pretty much the same question on the OpenCV website, but without an answer.
Well, I don't think anyone could tell you which parameter is what if you don't know the details of the algorithm that you are using. Besides, you should not need anyone to tell you which parameter is what if you know the details of the algorithm. I'm telling this for detailed parameters (fCT, fVarMax, etc.) not for straightforward ones (nmixtures, nShadowDetection, etc.).
So, I think you should read the papers referenced in the documentation. Here are the links for the papers 1, 2, 3.
And also you should read this paper as well, which is the beginning of background estimation.
After reading these papers and checking out the code with, I'm sure you will understand what those parameters are.
Good luck!
I have mat with only one column and 1600 rows. I want to filter it using a Gaussian.
I tried the following:
Mat AFilt=Mat(palm_contour.size(),1,CV_32F);
GaussianBlur(A,AFilt,cv::Size(20,1),3);
But I get the exact same values in AFilt (the filtered mat) and A. It looks like GaussianBlur has done nothing.
What's the problem here? How can I smooth a single-column mat with a Gaussian kernel?
I read about BaseColumnFilt, but haven't seen any usage examples so I'm not sure how to use them.
Any help given will be greatly appreciated as I don't have a clue.
I'm working with OpenCV 2.4.5 on windows 8 using Visual Studio 2012.
Thanks
Gil.
You have a single column but you are specifying the width of the gaussian to be big instead of specifying the height! OpenCV use row,col or x,y notation depending on the context. A general rule is whenever you use Point or Size, they behave like x,y and whenever the parameters are separate values they behave like row,col.
The kernel size should also be odd. If you specify the kernel size you can set sigma to zero to let OpenCV compute a suitable sigma value.
To conclude, this should work better:
GaussianBlur(A,AFilt,cv::Size(1,21),0);
The documentation og GaussianBlur says the kernel size must be odd, I would try using an odd size kernel and see if that makes any difference
I was studying Perlin's Noise through some examples # http://dindinx.net/OpenGL/index.php?menu=exemples&submenu=shaders and couldn't help to notice that his make3DNoiseTexture() in perlin.c uses noise3(ni) instead of PerlinNoise3D(...)
Now why is that? Isn't Perlin's Noise supposed to be a summation of different noise frequencies and amplitudes?
Qestion 2 is what does ni, inci, incj, inck stand for? Why use ni instead of x,y coordinates? Why is ni incremented with
ni[0]+=inci;
inci = 1.0 / (Noise3DTexSize / frequency);
I see Hugo Elias created his Perlin2D with x,y coordinates, and so does PerlinNoise3D(...).
Thanks in advance :)
I now understand why and am going to answer my own question in hopes that it helps other people.
Perlin's Noise is actually a synthesis of gradient noises. In its production process, we must compute the dot product of a vector pointing from one of the corners flooring the input point to the input point itself with the random-generated gradient vector.
Now if the input point were a whole number, such as the xyz coordinates of a texture you want to create, the dot product would always return 0, which would give you a flat noise. So instead, we use inci, incj, inck as an alternative index. Yep, just an index, nothing else.
Now returning to question 1, there are two methods to implement Perlin's Noise:
1.Calculate the noise values separately and store them in the RGBA slots in the texture
2.Synthesize the noises up before-hand and store them in one of the RGBA slots in the texture
noise3(ni) is the actual implementation of method 1, while PerlinNoise3D(...) suggests the latter.
In my personal opinion, method 1 is much better because you have much more flexibility over how you use each octave in your shaders.
My guess on the reason for using noise3(ni) in make3DNoiseTexture() instead if PerlinNoise3D(...) is that when you use that noise texture in your shader you want to be able to replicate and modify the functionality of PerlinNoise3D(...) directly in the shader.
My guess for the reasoning behind ni, inci, incj, inck is that using x,y,z of the volume directly don't give a good result so by scaling the the noise with the frequency instead it is possible to adjust the resolution of the noise independently from the volume size.