CN109214993B - Visual enhancement method for intelligent vehicle in haze weather - Google Patents
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Abstract
The invention discloses a visual enhancement method for an intelligent vehicle in haze weather, which comprises the following steps: 1) converting an image from an RGB color space to an HSV color space; 2) evaluating haze concentration; 3) calculating atmospheric coverage parameters; 4) obtaining a foreground image Ivis(x) (ii) a 5) Acquiring the current haze concentration as a background image by using a guiding filtering algorithm of a brightness channel, removing image noise by using a Gaussian filter, and increasing the influence of atmosphere coverage parameters on a foreground image; 6) according to step 5), the visual enhancement result is output. The invention can effectively improve the contrast and definition of the video, has higher calculation efficiency, effectively improves the image quality of the video signal, and improves the sensitivity, thereby ensuring the safety and the comfort of unmanned control.
Description
Technical Field
The invention relates to the field of visual enhancement, in particular to a visual enhancement method for an intelligent vehicle in haze weather.
Background
Current on-road computer vision systems are very sensitive to weather conditions, among which haze weather conditions are one of the most visually-critical of the various weather conditions. Under the haze weather condition, visibility is greatly reduced, visibility of a road environment system is poor, the obtained image is seriously degraded, blurring and contrast are reduced, serious color deviation and distortion can occur, many characteristics contained in the image are covered, the application value of the image is greatly reduced, and the visual systems cannot normally work.
In recent years, the sharpening processing of images in haze days has become a research hotspot in the fields of computer vision and image processing, attracts a large number of researchers at home and abroad, and has a plurality of methods proposed. However, due to the complexity and randomness of weather conditions, some algorithms proposed at present have certain limitations, and some research results and research methods obtained are still in continuous development and still need to be further improved and improved. In the prior art, a relatively effective haze weather image enhancement method is not found for the degradation problem of the image collected in the haze weather of the road vision system, so that the image enhancement can be effectively realized in the haze weather, the image quality of a video signal is improved in an effect increasing manner, and the sensitivity is improved.
Disclosure of Invention
In view of the above-mentioned defects in the prior art, the technical problem to be solved by the present invention is to provide an intelligent vehicle machine vision enhancement algorithm based on guided filtering. The method can effectively improve the image quality of the video signal and improve the sensitivity, thereby ensuring the safety and comfort of unmanned control.
In order to achieve the purpose, the invention provides a visual enhancement method for an intelligent vehicle in haze weather, which is characterized by comprising the following steps of: the method comprises the following steps:
1) converting an image from an RGB color space to an HSV color space;
2) evaluating haze concentration;
3) calculating atmospheric coverage parameters;
4) obtaining a foreground image Ivis(x);
5) Acquiring the current haze concentration as a background image by using a guiding filtering algorithm of a brightness channel, removing image noise by using a Gaussian filter, and increasing the influence of atmosphere coverage parameters on a foreground image;
6) according to step 5), the visual enhancement result is output.
Further, in the step 2), the haze concentration is calculated according to the following steps:
21) the evaluation factor of haze concentration is defined according to the following formula:
wherein D isdarkIs a dark channel prior;
u, v is the Fourier transform of the image pixel (x, y);
vdark(x, y) is that one of the at least three RGB color channels of pixel (x, y) has a lowA pixel value;
22) the haze concentration was calculated according to the following formula:
fβ=k×Ddark
where k is a linear scaling factor;
in order to ensure a non-distorted image, fβIs the haze concentration; f. ofβThe limited range of parameters is limited to [2,8]]。
Further, in the step 3), a current atmosphere coverage parameter is evaluated by using a guided filtering algorithm.
Further, calculating the atmosphere coverage parameter according to the following steps:
321) the kernel of the linear filter is built according to the following formula:
wherein, wkIs the kth kernel window; (a)k,bk) Is a linear transformation coefficient within a given cell window; i is a pixel index within the window; q. q.siIs an output image;
322) the subtle differences between the input image p and the output image q are distinguished according to the following formula:
wherein p isiIs an input image; q. q.siIs an output image;
323) calculating a solution of equation (12) according to the following equation;
wherein the luminance guide image I is taken to be equal to the input image p;
where ε is the regularized smoothing factor; covk(I, p) is that the guide map I and the input image are covariance matrixes; vark(I) Is the variance matrix of the guide map I;is the mean of the input image;is the mean of the guide graph I; ε is the smoothing factor.
324) Applying the guided filtering to the whole image region on the basis of retaining the hierarchical structure of the original image, and calculating an atmospheric coverage parameter I according to the following formula∞:
Where | w | is the number of pixels in the kernel window; m is the index number of the pixel; p is a radical ofmIs a pixel of the input image; w is amIs a reaction of with pmA kernel window for the center pixel;refers to the processing step of each pixel.
Further, in the step 4), a foreground image I is obtained according to the following formulavis(x):
Ivis(x)=E-I∞ (18)
Where E is atmospheric light at infinity.
The invention has the beneficial effects that: the invention provides a haze video enhancement algorithm based on a guide filtering method in order to improve low visibility and poor contrast of a vehicle-mounted video. First, the atmospheric attenuation model is simplified. Then, haze concentration is evaluated based on a dark prior theory. And then, acquiring the current haze concentration as a background image by using a guiding filtering algorithm of a brightness channel, and increasing the influence of atmosphere coverage parameters on the foreground image. The method can effectively improve the contrast and definition of the video, has higher calculation efficiency, effectively improves the image quality of the video signal, and improves the sensitivity, thereby ensuring the safety and the comfort of driving and controlling in haze weather.
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FIG. 1 is a flow chart illustrating the steps of one embodiment of the present invention.
Detailed Description
The invention is further illustrated by the following examples in conjunction with the accompanying drawings:
as shown in fig. 1, the method for enhancing the vision of the intelligent vehicle in the haze weather comprises the following steps:
1) converting an image from an RGB color space to an HSV color space;
2) evaluating haze concentration;
3) calculating atmospheric coverage parameters;
4) obtaining a foreground image Ivis(x);
5) The current haze concentration is obtained by using a guiding filtering algorithm of a brightness channel and is used as a background image, image noise is removed by using a Gaussian filter, and the influence of atmosphere coverage parameters on a foreground image is increased.
6) According to step 5), the visual enhancement result is output.
He, according to the dark prior theory of dr, indicates that a sharp image has low pixel values in one of at least three RGB color channels, which can be expressed as:
Jdark(x)=min(min(Jc(y)))c∈{r,g,b},y∈Ω(x) (9)
here, JcIs the color channel of the RGB image J; Ω (x) is the statistical region where x is off center.
JdarkAre always small, even close to zero, and, in sharp images,except for a large number of clear image statistical analyses in sky regions. The dark tone image and the image under different haze concentrations are compared, and the average pixel gray scale of the dark tone image can be found through the darker tone partial image so as to be used for evaluating the haze concentration of the current environment.
Therefore, in particular, in the step 2), the haze concentration is calculated according to the following steps:
21) the evaluation factor of haze concentration is defined according to the following formula:
wherein D isdarkIs a dark channel prior;
u, v is the Fourier transform of the image pixel (x, y);
vdark(x, y) is that one of the at least three RGB color channels of pixel (x, y) has a low pixel value;
22) the haze concentration was calculated according to the following formula:
fβ=k×Ddark
where k is a linear scaling factor; f. ofβIs the concentration of the haze,
to ensure a non-distorted image, the limited range of parameters is defined as [2,8 ].
In particular, in the step 3), the current atmosphere coverage parameter is evaluated by using a guided filtering algorithm.
In particular, the calculation of the atmospheric coverage parameter is carried out according to the following steps:
321) the kernel of the linear filter is built according to the following formula:
wherein, wkIs the kth kernel window; (a)k,bk) Is a linear transformation coefficient within a given cell window; i is a pixel index within the window; q. q.siIs an output image;
322) the subtle differences between the input image p and the output image q are distinguished according to the following formula:
wherein p isiIs an input image; q. q.siIs an output image;
323) calculating a solution of equation (12) according to the following equation;
wherein the luminance guide image I is taken to be equal to the input image p;
where ε is the regularized smoothing factor; covk(I, p) is that the guide map I and the input image are covariance matrixes; vark(I) Is the variance matrix of the guide map I;is the mean of the input image;is the mean of the guide graph I; ε is the smoothing factor.
324) Applying the guided filtering to the whole image region on the basis of retaining the hierarchical structure of the original image, and calculating an atmospheric coverage parameter I according to the following formula∞:
Where | w | is the number of pixels in the kernel window; m is the index number of the pixel; p is a radical ofmIs a pixel of the input image; w is amIs a reaction of with pmA kernel window for the center pixel;refers to the processing step of each pixel. In this embodiment, the smoothing factor epsilon is set to 0.3, in other embodiments, the smoothing factor can also be set according to different requirements to achieve the same technical effect, and the width r of the kernel window is set to 30 pixel points.
Specifically, in the step 4), the foreground image I is obtained according to the following formulavis(x):
Ivis(x)=E-I∞(18) Wherein E is atmospheric light at infinity
With regard to the selection of filters, most computer vision and computer graphics image filtering currently involves suppressing or extracting the content of the image. Simple nucleated linear translation invariant filters (LTI), such as average, gaussian, laplacian, and Sobel filters, are widely used for image restoration, blurring/sharpening, edge detection, feature extraction, and so on. Alternatively, LTI filters can explicitly perform image stitching, image matting, and gradient domain operations by solving a poisson equation compressed at High Dynamic Range (HDR), with filter kernels explicitly defined by the transpose of a homogeneous laplace matrix.
The LTI filtering kernel is spatially invariant and independent of the image content, but usually sometimes needs to take into account additional information that leads to the image. The precursor work of the anisotropic diffusion guides the diffusion process by the gradient of the image to be filtered, and the phenomenon that the image is smoothed to the edge is avoided. The sum of squares minimum weighting filter uses the input image to be filtered to guide and selects a quadratic function that is equivalent to the anisotropic diffusion of a non-normal stable state. In other applications, the guide image can also be another image than the input image from the moment. The guided filter output results in a local linear transformation of the guided image. On the one hand, the steering filter has a good edge-preserving smoothing effect, like the bilateral filter, but it does not have the effect of gradient inversion artifacts. On the other hand, the guided filtering can be much more than just smooth, which allows the filtering output to be more structured and less smooth than the input with the aid of a guided graph.
In the technical scheme, the selected guiding filtering is mainly realized by the following modes:
we first define a generic linear translation transform filter routine, associated with the guide image I, a filtered input image P and an output image q. I and p are given in advance according to the application and they may be identical. The result of the filtering at a pixel i is expressed as a weighted average:
where i and j are both pixel indices. The filter kernel Wij is a function that directs the image I and is independent of p. This filter is linearly related to p.
An example of one such filter is a cascaded filter and the bilateral filtering kernel Wbf is given by the following equation:
wherein X is the pixel coordinate; ki is a normalization parameter ensuring that sigma jWijbf is 1; parameter sigmasAnd σrAnd respectively adjusting the sensitivity of the spatial similarity and the color brightness range similarity. When P and I are equal, the cascaded filter degrades into an initial bilateral filter.
The explicit weighted average filter optimizes a quadratic function and solves a linear system of equations of the form:
Aq=P (3)
q and p are the column vectors N-1, respectively { qi } and { pi }; a is an N-N matrix associated only with I. The solution q of formula (3) is a-1p, and has the same form as (1), and Wij is (a-1) ij.
We now define a guided filter, the key assumption being that this guided filter is a locally linear model between the guided image I and the filtered output q. We assume that q is a linear transformation of I centered in the window Wk of pixel k:
(ak, bk) is a square window of radius r, assuming the same linear coefficient as Wk. This local linear model determines that if I has an edge, then q has an edge because
In order to determine the linear coefficients (ak, bk), the input filtered image P needs to be constrained. We define the output q as the input p minus some undesired content n, e.g. noise/texture:
qi=pi-ni (5)
we sought a solution that minimizes the difference between q and p while maintaining a linear model (4). In particular, we minimize the cost function of the following window Wk:
here, e is a regularization parameter that penalizes large ak.
Equation (6) is a linear ridge regression model, which is solved by equation (7) given below:
here,. mu.kAndis the window Wk mean and variance of the guide image I; i W is the number of pixels in Wk;
is the average value of P over Wk. Linear coefficients (ak, bk) are obtained and we can compute the filtered output qi root.
However, one pixel i is associated with all overlapping windows Wk covering i, so the value of qi in equation (5) is not the same but is calculated in different windows. One simple strategy is to average all possible values of qi. Therefore, the (ak, bk) values of Wk windows in all images are computed, and we compute the output by filtering:
This overlapping window averaging strategy is popular in image denoising and is very successful.
Equations (6), (7), (8) are definitions of the steering filter.
By adopting the guiding filtering, the technical scheme simplifies the atmospheric attenuation model. And evaluating the haze concentration based on a dark prior theory, then obtaining the current haze concentration as a background image by utilizing a guide filtering algorithm of a brightness channel, and increasing the influence of atmosphere coverage parameters on the foreground image. The method provided by the invention can effectively improve the contrast and definition of the video and has higher calculation efficiency.
The foregoing detailed description of the preferred embodiments of the invention has been presented. It should be understood that numerous modifications and variations could be devised by those skilled in the art in light of the present teachings without departing from the inventive concepts. Therefore, the technical solutions available to those skilled in the art through logic analysis, reasoning and limited experiments based on the prior art according to the concept of the present invention should be within the scope of protection defined by the claims.
Claims (3)
1. A haze weather intelligent vehicle vision enhancement method is characterized by comprising the following steps: the method comprises the following steps:
1) converting an image from an RGB color space to an HSV color space;
2) evaluating haze concentration;
3) calculating atmospheric coverage parameter I∞;
4) Obtaining a foreground image Ivis(x),Ivis(x)=E-I∞Where E is atmospheric light at infinity;
5) acquiring the current haze concentration as a background image by using a guiding filtering algorithm of a brightness channel, removing image noise by using a Gaussian filter, and increasing the influence of atmosphere coverage parameters on a foreground image;
in the step 2), the haze concentration is calculated according to the following steps:
21) the evaluation factor of haze concentration is defined according to the following formula:
wherein D isdarkIs a dark channel prior;
uxv is the Fourier transform of the image pixel (x, y);
vdark(x, y) is that one of the at least three RGB color channels of pixel (x, y) has a low pixel value;
22) the haze concentration was calculated according to the following formula:
fβ=k×Ddark
where k is a linear scaling factor; wherein f isβIs the haze concentration;
to ensure a non-distorted image, fβThe limited range of parameters is defined as [2,8]]。
2. The haze weather intelligent vehicle vision enhancement method as claimed in claim 1, wherein: in the step 3), the current atmosphere coverage parameter is evaluated by using a guided filtering algorithm.
3. The haze weather intelligent vehicle vision enhancement method as claimed in claim 2, wherein:
in the step 3), calculating the atmosphere coverage parameter according to the following steps:
321) the kernel of the linear filter is built according to the following formula:
wherein, wkIs the kth kernel window; (a)k,bk) Is a linear transform coefficient within a given unit window; i is a pixel index within the window; q. q.siIs an output image; i isiIs the intensity of the observed image;
322) the subtle differences between the input image p and the output image q are distinguished according to the following formula:
wherein p isiIs an input image; q. q.siIs an output image;
323) calculating a solution of equation (12) according to the following equation;
wherein the luminance guide image I is taken to be equal to the input image p;
where ε is the regularized smoothing factor; covk(I, p) is the covariance matrix of the guide map I and the input image; vark(I) Is the variance matrix of the guide map I;is the mean of the input image;is the mean of the guide graph I;
324) applying guided filtering to the whole image area on the basis of preserving the hierarchical structure of the original image, and calculating an atmospheric coverage parameter I according to the following formula∞:
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