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2021-02-10 19:30
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2021年2月10日发(作者:depressed)


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A


3 Image Enhancement in the Spatial Domain


The principal objective of enhancement is to process an image so that the result


is more suitable than the original image for a specific application. The word specific


is important, because it establishes at the outset than the techniques discussed in this


chapter


are


very


much


problem


oriented.


Thus,


for


example,


a


method


that


is


quite


useful


for


enhancing


X-ray


images


may


not


necessarily


be


the


best


approach


for


enhancing pictures of Mars transmitted by a space probe. Regardless of the method


used


.However,


image


enhancement


is


one


of


the


most


interesting


and


visually


appealing areas of image processing.


Image


enhancement


approaches


fall


into


two


broad


categories:


spatial


domain


methods and frequency domain methods. The term spatial domain refers to the image


plane itself, and approaches in this category are based on direct manipulation of pixels


in


an


image.


Fourier


transform


of


an


image.


Spatial


methods


are


covered


in


this


chapter, and frequency domain enhancement is discussed in Chapter ement


techniques based on various combinations of methods from these two categories are


not unusual. We note also that many of the fundamental techniques introduced in this


chapter in the context of enhancement are used in subsequent chapters for a variety of


other image processing applications.


There is no general theory of image enhancement. When an image is processed


for


visual


interpretation,


the


viewer


is


the


ultimate


judge


of


how


well


a


particular


method


works.


Visual


evaluation


of


image


quality


is


a


highly


is


highly


subjective


process, thus making the definition of a “good image” an elusive standard by which to


compare algorithm performance. When the problem is one of processing images for


machine perception, the evaluation task is somewhat easier. For example, in dealing


with


a


character


recognition


application,


and


leaving


aside


other


issues


such


as


computational


requirements,


the


best


image


processing


method


would


be


the


one


yielding


the


best


machine


recognition


results.


However,


even


in


situations


when


a


clear-cut criterion of performance can be imposed on the problem, a certain amount of


trial and error usually is required before a particular image enhancement approach is


selected.


3.1 Background


As indicated previously, the term spatial domain refers to the aggregate of pixels


composing an image. Spatial domain methods are procedures that operate directly on


these pixels. Spatial domain processes will be denotes by the expression


g


?


x


,


y


?


?


T


?

< br>f


(


x


,


y


)


?















(3.1-1)


where


f(x,


y)


is


the


input


image,


g(x,


y)


is


the


processed


image,


and


T


is


an


operator on f, defined over some neighborhood of (x, y). In addition, T can operate on


a


set


of


input


images,


such


as


performing


the


pixel-by-pixel


sum


of


K


images


for


noise reduction, as discussed in Section 3.4.2.


The principal approach in defining a neighborhood about a point (x, y) is to use a


square or rectangular subimage area centered at (x, y).The center of the subimage is


moved from pixel to starting, say, at the top left corner. The operator T is applied at


each location (x, y) to yield the output, g, at that location. The process utilizes only


the


pixels


in


the


area


of


the


image


spanned


by


the


neighborhood.


Although


other


neighborhood shapes, such as approximations to a circle, sometimes are used, square


and


rectangular


arrays


are


by


far


the


most


predominant


because


of


their


ease


of


implementation.


The simplest from of T is when the neighborhood is of size 1×


1 (that is, a single


pixel).


In


this


case,


g


depends


only


on


the


value


of


f


at


(x,


y),


and


T


becomes


a


gray- level (also called an intensity or mapping) transformation function of the form


s


?


T


(


r


)



























(3.1-2)


where, for simplicity in notation, r and s are variables denoting, respectively, the


grey level of f(x, y) and g(x, y)at any point (x, y).Some fairly simple, yet powerful,


processing


approaches


can


be


formulates


with


gray-level


transformations.


Because


enhancement at any point in an image depends only on the grey level at that point,


techniques in this category often are referred to as point processing.


Larger neighborhoods allow considerably more flexibility. The general approach


is


to


use


a


function


of


the


values


of


f


in


a


predefined


neighborhood


of


(x,


y)


to


determine the value of g at (x, y). One of the principal approaches in this formulation


is based on the use of so-called masks (also referred to as filters, kernels, templates, or


windows). Basically, a mask is a small (say, 3×


3) 2-Darray, in which the values of the


mask coefficients determine the nature of the type of approach often are referred to as


mask processing or filtering. These concepts are discussed in Section 3.5.


3.2 Some Basic Gray Level Transformations


We begin the study of image enhancement


techniques by discussing gray-level


transformation


functions.


These


are


among


the


simplest


of


all


image


enhancement


techniques. The values of pixels, before and after processing, will be denoted by r and


s,


respectively.


As


indicated


in


the


previous


section,


these


values


are


related


by


an


expression of the from s = T(r), where T is a transformation that maps a pixel value r


into


a


pixel


value


s.


Since


we


are


dealing


with


digital


quantities,


values


of


the


transformation


function


typically


are


stored


in


a


one-dimensional


array


and


the


mappings from r to s are implemented via table lookups. For an 8-bit environment, a


lookup table containing the values of T will have 256 entries.


As an introduction to gray-level transformations, which shows three basic types


of


functions


used


frequently


for


image


enhancement:


linear


(negative


and


identity


transformations),


logarithmic


(log


and


inverse-log


transformations),


and


power-law


(nth power and nth root transformations). The identity function is the trivial case in


which out put intensities are identical to input intensities. It is included in the graph


only for completeness.


3.2.1 Image Negatives


The


negative


of


an


image


with


gray


levels


in


the


range


[0,


L-1]is


obtained


by


using the negative transformation show shown, which is given by the expression


s


?


L


?


1


?


r

< p>






















(3.2-1)



Reversing


the


intensity


levels


of


an


image


in


this


manner


produces


the


equivalent of a photographic negative. This type of processing is particularly suited


for enhancing white or grey detail embedded in dark regions of an image, especially


when the black areas are dominant in size.



3.2.2 Log Transformations


The general from of the log transformation is


s


?


c


log(1


?


r


)






















(3.2-2)



Where c is a


constant, and it is assumed that r ≥0 .The shape of the log curve


transformation maps a narrow range of low gray-level values in the input image into a


wider range of output levels. The opposite is true of higher values of input levels. We


would


use


a


transformation


of


this


type


to


expand


the


values


of


dark


pixels


in


an


image while compressing the higher- level values. The opposite is true of the inverse


log transformation.


Any curve having the general shape of the log functions would accomplish this


spreading/compressing


of


gray


levels


in


an


image.


In


fact,


the


power- law


transformations discussed in the next section are much more versatile for this purpose


than the log transformation. However, the log function has the important characteristic


that


it


compresses


the


dynamic


range


of


image


characteristics


of


spectra.


It


is


not


unusual


to


encounter


spectrum


values


that


range


from


0


to


106


or


higher.


While


processing numbers such as these presents no problems for a computer, image display


systems


generally


will


not


be


able


to


reproduce


faithfully


such


a


wide


range


of


intensity values .The net effect is that a significant degree of detail will be lost in the


display of a typical Fourier spectrum.


3.2.3 Power-Law Transformations


Power-Law transformations have the basic from


s


?


cr


?

























(3.2-3)



Where c and y are positive constants .Sometimes Eq. (3.2-3) is written as




to


account for an offset (that is, a measurable output when the input is zero). However,


offsets typically are an issue of display calibration and as a result they are normally


ignored in Eq. (3.2-3). Plots of s versus r for various values of y are shown in Fig.3.6.


As in the case of the log transformation, power-law curves with fractional values of y


map a narrow range of dark input values into a wider range of output values, with the


opposite being true for higher values of input levels. Unlike the log function, however,


we notice here a family of possible transformation curves obtained simply by varying


y.


As


expected,


we


see


in


Fig.3.6


that


curves


generated


with


values


of


y



1


have


exactly the opposite effect as those generated with values of


y



1. Finally, we note


that Eq.(3.2-3) reduces to the identity transformation when c = y = 1.


A


variety


of


devices


used


for


image


capture,


printing,


and


display


respond


according to as gamma[hence our use of this symbol in Eq.(3.2-3)].The process used


to correct this power-law response phenomena is called gamma correction.


Gamma correction is important if displaying an image accurately on a computer


screen is of concern. Images that are not corrected properly can look either bleached


out,


or,


what


is


more


likely,


too


dark.


Trying


to


reproduce


colors


accurately


also


requires some knowledge of gamma correction because varying the value of gamma


correcting changes not only the brightness, but also the ratios of red to green to blue.


Gamma correction has become increasingly important in the past few years, as use of


digital


images


for


commercial


purposes


over


the


Internet


has


increased.


It


is


not


Internet has increased. It is not unusual that images created for a popular Web site will


be viewed by millions of people, the majority of whom will have different monitors


and/or monitor settings. Some computer systems even have partial gamma correction


built in. Also, current image standards do not contain the value of gamma with which


an image was created, thus complicating the issue further. Given these constraints, a


reasonable approach when storing images in a Web site is to preprocess the images


with a gamma that represents in a Web site is to preprocess the images with a gamma


that represents an “average” of the types of monitors and computer systems that one


expects in the open market at any given point in time.


3.2.4 Piecewise-Linear Transformation Functions


A


complementary


approach


to


the


methods


discussed


in


the


previous


three


sections


is


to


use


piecewise


linear


functions.


The


principal


advantage


of


piecewise


linear functions over the types of functions we have discussed thus far is that the form


of


piecewise


functions


can


be


arbitrarily


complex.


In


fact,


as


we


will


see


shortly,


a


practical


implementation


of some important


transformations can be formulated only

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