mip1_02_camera_systems_090505_1436383

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Unformatted text preview: Medical Image Processing 1 (MIP1) Image Signal Analysis and Processing (ISAP) SS’09 Camera Systems Dr. Pierre Elbischger School of Medical Information Technology Carinthia University of Applied Sciences Lightning Technology (Overview) •Reflected (1) vs. transmitted (2) light: (1) light source positioned in front of object (2) light source positioned behind object • Bright field (1) vs. dark field (2): specular reflection of a surface patch parallel to the optical axis reach the lens aperture (bright field) or do not reach the lense aperture (dark field) •Coaxial light illuminates the object frontal. This can be realized by means of prisms or so called ring lights fixated around the camera’s objective. Ring lights usually consist of several LED elements. Different lightning technologies [1] 05.05.2009 Dr. Pierre Elbischger - Camera Systems - MIP1/ISAP'SS09 2 Lightning Technology (Examples) Bright field [1] Dark field [1] •Using dark field light the lightning situation is inverted. Flat regions appear dark while stampings, scratches and grooves are seen clearly. Bright field [1] Coaxial ring light [1] By means of coaxial lightning unwanted shadows can be avoided. 05.05.2009 Dr. Pierre Elbischger - Camera Systems - MIP1/ISAP'SS09 3 Optics Besides the lightning the imaging optic or camera objective plays an important role in the image acquisition process. Depending on the scene an appropriate objective must be chosen. In the following relevant objective characteristics as well as deducible parameters are introduced. manufacturer Pentax type designation TV Lens H1214-M description Manually controlled high-resolution objective for 2 Megapixel C- and CS-Mount cameras interface, sensor size C-Mount, ½” focal length 12mm aperture range F 1.4 – 16 aperture control manual, fixable focus control manual, fixable angle of field horiz. ~ 29.8° min. object distance 0.25m Parameters of a C-Mount Pentax objective [1] 05.05.2009 Dr. Pierre Elbischger - Camera Systems - MIP1/ISAP'SS09 4 Objective Interfaces In general two standardized objective mounting parts are distinguished: C-Mount and CS-Mount. Both have a diameter of one inch (25.4mm) and a thread pitch of 1/32 inch (32 turns per inch). The flange back (distance between objective contact surface and image plane, Auflagemaß) is 17.5mm with C-Mount and 12.5mm with CS-Mount. C-/CS-Mount-flange backs and their possible combination with an AVT CS-Mount-camera [1] Adding a 5mm spacer ring, a C-Mount-objective may also be used with a CS-Mountcamera. In contrast, a CS-Mount-objective may never be used with a C-Mount-camera. Besides, there exist several more adapters that allow for combining other objectives with C-Mount-cameras. 05.05.2009 Dr. Pierre Elbischger - Camera Systems - MIP1/ISAP'SS09 5 Formats •The size describes the dimensions of the image sensor within a camera. In the data sheet of an objective, the largest sensor size that can be used is stated – it is possible to used sensor chips with less or equal size. Combining a large-sized objective with a smaller image sensor is often even beneficial because the more distorted outer area of the lens has no contribution to the image formation. m m Attention The given diagonal values don’t match the effective sensor size. Rather they are a relict of the tube cameras and correspond to the exterior diameter of the camera tube. Common image sensor size for the C-Mount standard [1] 05.05.2009 m m Dr. Pierre Elbischger - Camera Systems - MIP1/ISAP'SS09 6 The pinhole camera (1) • The image is formed by light rays issued from the scene facing the box. • If the pinhole is reduced to a point (theoretically), exactly one ray of light would pass the pinhole and contribute to a single point in the image. • A pinhole of finite size would collect light from a cone of rays, subtending a finite solid angle, in a single point on the image plane and result in blurry images. • The object points are related to the image points by a perspective projection optical axis pinhole image plain 05.05.2009 Dr. Pierre Elbischger - Camera Systems - MIP1/ISAP'SS09 7 The pinhole camera II • • • The larger the pinhole, the brighter the image, but a large pinhole gives blurry images. Shrinking the pinhole produces sharper images, but reduces the amount of light reaching the image plane and may introduce diffraction effects. Diffraction occurs if the diameter of the aperture is in the order of the wavelength of the used light. Diffraction pattern of a small circular pinhole. 05.05.2009 Dr. Pierre Elbischger - Camera Systems - MIP1/ISAP'SS09 8 Thin lens • For two reasons the pinhole is replaced by a lens in most cameras: • Similar to the pinhole camera the lens leads to a perspective projection of the object onto the image plane. – – to gather light to keep the image sharp while gathering light from a large area. Refraction Reflection and refraction at the interface between two homogeneous media with indices of refraction n1 and n2 are by Snell’s law. Considering first-order (praxial) geometrics, where angles between all light rays going through a lens and the normal to the refractive surface of the lens are small, one can use the praxial refraction equation as an approximation of Descarts’ law. 05.05.2009 Dr. Pierre Elbischger - Camera Systems - MIP1/ISAP'SS09 9 Thin-Lense Equation (Focal Length) When choosing an objective, the required focal length depends on the given object distance g, the object size G and the image size B. To the object size G applies: Gwidth G= Gheight if Gwidth ≥ 1.33 ⋅ Gheight otherwise Path of rays on thin lenses1 for common 4:3 sensor formats (analog for image size B). From the theorem of intersecting lines the magnification V may be deduced1: 1Gg f === V B b b− f leading to the thin-lens equation of Descartes: 111 = +. f gb Inserting and transforming these equations one obtains the needed formula for the focal length: f= 1approximation 05.05.2009 g⋅B . G+B How focal length affects photograph composition: adjusting the camera's distance from the main subject while changing focal length, the main subject can remain the same size, while the other at a different distance changes size. when taking the thin lens model as basis the praxial refraction equation holds Dr. Pierre Elbischger - Camera Systems - MIP1/ISAP'SS09 10 Focal Length (Example) Example: The human eye (50x35mm²) shall be captured for a biometric access control (iris recognition) in a distance of 500mm using a 1/4” image sensor (3.2x2.4mm²). given values: G = 50mm B = 3.2mm g = 500mm seeked value: f solution: f= g ⋅ B 500 ⋅ 3.2 = = 30.07 mm G + B 50 + 3.2 To ensure that the entire object is contained in the image, an objective with a minimal wider angle (smaller focal length) is chosen. Besides, there exist standardized focal length graduations from which the best matching one is taken. f = 4.2, 6, 8, 9, 12, 16, 25, 35, 50, … [mm]. In the given example f = 25mm would do a good job. 05.05.2009 Dr. Pierre Elbischger - Camera Systems - MIP1/ISAP'SS09 11 Focusing Adjusting the focus of an objective corresponds to changing the image width b. Focusing an object being far away (g ∞), the image distance b converges to the focal length f. Focusing an object being quite close to the objective, the shortening of g is limited by the minimum object distance MOD (see next slides). Principle of focusing Similar to the aperture also the focus of an objective can be adjusted manually or motorized, whereas not all objectives have an adjustable focus at all. 05.05.2009 Dr. Pierre Elbischger - Camera Systems - MIP1/ISAP'SS09 12 Minimum Object Distance The Minimum Object Distance MOD is the minimum reasonable distance between the front lens and the object to be captured. For object distances smaller than MOD it is no more possible to bring the object into focus. The MOD is given by the limit stop of the objective’s focusing mechanism and can be varied by adding spacer rings (sr) between objective and camera. The equation for calculating the needed spacer ring size d for a given arrangement can be deduced from the thin lens equations (see before). MOD = g min , b= f ⋅ MOD , MOD − f MODsr = g sr,min = d = bsr − b = bsr = b + d 111 = +. f gb bsr ⋅ f bsr − f f ⋅ MODsr f ⋅ MODsr f ⋅ MOD f ⋅ MOD − = − MODsr − f MOD − f f − MOD f − MODsr The new magnification Vsr is given by: Vsr = bsr b − f d = + g sr f f ⇒ Vsr,max = V + d , Vsr,min = f 1Gg f === V B b b− f For g=∞ b converges to the focal length f and the d first term in the , equation vanishes. f V Due to the supposed thin lens assumption, in general these equations will give estimates rather than exact values. 05.05.2009 Dr. Pierre Elbischger - Camera Systems - MIP1/ISAP'SS09 13 Depth of Field (1) In optics, particularly as it relates to film and photography, the depth of field (DOF) is the portion of a scene that appears sharp in the image. Although a lens can precisely focus at only one distance, the decrease in sharpness is gradual on either side of the focused distance, so that within the DOF, the blurring is imperceptible under normal viewing conditions. Effect of aperture on blur and DOF. The points in focus (2) project points onto the image plane (5), but points at different distances (1 and 3) project blurred images, or circles of confusion. Decreasing the aperture size (4) reduces the size of the blur circles for points not in the focused plane, so that the blurring is imperceptible, and all points are within the DOF. An ideal point is projected as a circle of confusion into the image (point-spread-function). Using digital matrix cameras (i.e. CCD cameras) the diameter ∅ of the circle of confusion shouldn’t be larger than the size of a single pixel element. Otherwise image information is lost. ∅ = Min( pixel width , pixel height ) 05.05.2009 Dr. Pierre Elbischger - Camera Systems - MIP1/ISAP'SS09 14 Depth of Field (2) - The f-number In optics, the f-number N (sometimes called focal ratio, f-ratio or relative aperture) of an optical system expresses the diameter of the entrance pupil D in terms of the effective focal length f of the lens; in simpler terms, the f-number is the focal length divided by the aperture diameter. The amount of light captured by a lens is proportional to the area of the aperture A. Modern lenses use a standard f-stop scale, which is an approximately geometric sequence of numbers (index n=0,1,2,…) that corresponds to the sequence of the powers of √2=1.414: f1, f1.4, f2, f2.8, f4, f5.6, f8, f11, f16, f22, f32, f45, f64, f90, f128, etc. The values of the ratios are rounded off to these particular conventional numbers, to make them easy to remember and write down. Thus, two consecutive steps in the f-number sequence correspond to a reduction in light intensity by a factor of two (half area A). Reducing the aperture size (increasing the f-number): reduce the amount of light passing the aperture may require an increase of the exposure time increases the depth-of-field 05.05.2009 Dr. Pierre Elbischger - Camera Systems - MIP1/ISAP'SS09 Sequence of f-numbers 15 Depth of Field (3) The pixel size can either be calculated from the pixel number and the sensor dimensions or it can be taken from the sensor’s data sheet. A typical pixel size of a modern camera sensors is 5x5µm. The front lf and back lb depth of field limits along the optical axis can be calculated as followed: l f ,b = To the depth of field range r applies: g− f 1± ∅ ⋅ N ⋅ 2 f r = lb − l f = According to the equation, the focal length f as well as the f-number N influence the depth of field. In order to increase the depth of field a higher f-number can be chosen (smaller aperture). For g>>f the focal length has an approximately quadratic influence and, thus, it’s useful to use a wide angle objective (smaller focal length) to increase the depth of field. 05.05.2009 g . g g− f 1− ∅ ⋅ N ⋅ 2 f f-number: 5.6 Dr. Pierre Elbischger - Camera Systems - MIP1/ISAP'SS09 − g g− f 1+ ∅ ⋅ N ⋅ 2 f . f-number: 22 16 Angle of Field The specification of the angle of field Θ is redundant to the specification of the focal length f and the sensor format Bmax. Θ = 2 ⋅ arctan Bmax 2f Even though the information is redundant, the angle of field is often added to the data sheet. Thus, the angle of field easily allows for assessing the kind or type of an objective. Commonly one distinguishes wide-angle- (Θ>50 ), standard- (Θ≈50 ) or telephoto-lenses (Θ<50 ). Example: For the format of a classical (analog) consumer camera (24x36mm², diagonal 43.2mm) one obtains a focal length f = 50mm for the standard objective. For a 1/4” sensor a focal length of f = 5mm is obtained for the same objective. In both cases the image diagonal was used in the calculation. 05.05.2009 Dr. Pierre Elbischger - Camera Systems - MIP1/ISAP'SS09 17 Extended depth-of-field (EDoF) Image series of out-of-focus images (large microscopy magnification) Image processing algorithms can be used to create one image of an extend depth-of-field from a series of images that are partially out of focus. 05.05.2009 Extended depth-of-field image Dr. Pierre Elbischger - Camera Systems - MIP1/ISAP'SS09 20 Real lens - Aberrations • • A more realistic model of simple optical systems is the thick lens. Simple lenses suffer from a number of aberrations. Plane of least confusion Spherical aberration The praxial refraction equation was only an approximation (the first order term of a Taylor expansion). Using higher order terms one can show that rays striking the interface farther from the optical axis are focused closer to the interface. Distortion This effect is due to the fact that different areas of a lens have slightly different focal lengths. Chromatic aberration The index of refraction of a transparent medium depends on the wavelength (color) of the incident light rays. 05.05.2009 Dr. Pierre Elbischger - Camera Systems - MIP1/ISAP'SS09 21 Compound lenses • Aberrations can be minimized by aligning several simple lenses with well-chosen shapes and refraction indices, separated by appropriate stops. • These compound lenses can still be modeled by the thick lens equation. 05.05.2009 Dr. Pierre Elbischger - Camera Systems - MIP1/ISAP'SS09 22 Vignetting • The complex compound (correction) lenses still suffer from one more defect relevant to image processing called vignetting. • Vignetting is caused by light beams emanating from object points located off axis that are partially blocked by various apertures positioned inside the lens to limit aberrations. This phenomenon causes the irradiance to drop in the image periphery. • Because of other reasons irradiance is also proportional to cos4(α) and falls off as the light rays deviate from the optical axis. In typical situations this term can be neglected. Vignetting effect in a two-lens system 05.05.2009 Vignetting as it appears in images Dr. Pierre Elbischger - Camera Systems - MIP1/ISAP'SS09 23 CCD cameras • • • • A CCD sensor is placed in the image plane of the optical system The CCD sensor consists of an regular (matrix) array of photo diodes that collect electrons that are created by the photo electrical effect as light shines onto the photo diode. The integrated charge in a photo diode cell is almost linear in time and light intensity. Under conditions where a CCD is exposed to very high intensity illumination, it is possible to exhaust the storage capacity of the CCD wells, a condition known as blooming. When this occurs, excess charge will overflow into adjacent CCD photodiode wells resulting in a corrupted image near the blooming site. The preferred blooming direction is the read-out direction of the CCD sensor. 05.05.2009 Dr. Pierre Elbischger - Camera Systems - MIP1/ISAP'SS09 24 CCD cameras The frame-transfer CCD. Uses a two-part sensor in which one-half of the parallel array is used as a storage region and is protected from light by a light-tight mask. • The interline-transfer CCD. Incorporates charge transfer channels called Interline Masks. These are immediately adjacent to each photodiode so that the accumulated charge can be rapidly shifted into the channels after image acquisition has been completed. The very rapid image acquisition virtually eliminates image smear. 05.05.2009 Dr. Pierre Elbischger - Camera Systems - MIP1/ISAP'SS09 Interline-Transfer • Frame-Transfer Full frame CCD. The accumulated charge must be shifted vertically row by row into the serial output register and for each row the serial output register must be shifted horizontally to readout each individual pixel (progressive scan). A disadvantage of full frame is charge smearing caused by light falling on the sensor whilst accumulated charge signal is being transferred to the readout register. Use a mechanical shutter to avoid smearing. Full frame • 25 Image digitization • • • To create a digitized image f(n,m), we need to convert the continues sensed data f(x,y) into digital form. Digitizing the coordinate values is called sampling (is performed by the CCD-chip). Digitizing the Amplitude values is called quantization. 05.05.2009 Dr. Pierre Elbischger - Camera Systems - MIP1/ISAP'SS09 26 Sampling / Resolution 05.05.2009 Dr. Pierre Elbischger - Camera Systems - MIP1/ISAP'SS09 27 Resolution •Considering the resolution one has to distinguish the sensor resolution Rcamera [pixel] and the spatial resolution Rspatial [mm/pixel] at the object, which are related by: Rcamera = G’ is the field of view [mm]. It consists of the object size G, a tolerance in the object position t and a safety value sf (usually 1.2). G' Rspatial •The spatial resolution is the size of the smallest resolvable feature s [mm] divided by the number of pixels npx [px] that it occupies in the image. Rspatial = s npx •With pixel accurate calculations npx=1px, applying sub-pixel methods (use interpolation, area moments, …) it results in npx=1/sub-pixel-factor. The following table shows typical values for various applications. method sub-pixel-factor with ideal conditions sub-pixel-factor in practice determining the center of gravity 10-20 4-8 camera calibration 6-10 2-6 object measurement 1 0.3 segmentation 6-10 2-6 pattern matching touching edges binary-large-object-analysis gray-value-correlation application Realizable sub-pixel-factors sorted by methods 05.05.2009 Dr. Pierre Elbischger - Camera Systems - MIP1/ISAP'SS09 28 Resolution: Example 1 For the given stamping part the marked distance between two borehole midpoints shall be measured. given values: G = 60mm (object width) t = 10mm (max positioning error) sf = 20mm (safety) s = 0.02mm (measuring accuracy) method: determination of the circles’ centers of gravity sub-pixel-factor (table): 4, npx = 1px/4 = 0.25px seeked value: Rcamera (camera resolution) solution: Rspatial = G ' = G + t + sf = 60mm + 10mm + 20mm = 90mm µm 0.02mm s = = 80 npx 0.25 px px Rcamera = G' Rspatial = 90mm = 1125 px 80 µm / px A standard resolution that is available is 1280x960px². 05.05.2009 Dr. Pierre Elbischger - Camera Systems - MIP1/ISAP'SS09 29 Resolution: Example 2 In example 1 an ideal objective with an arbitrary focal length f that realizes G’=90mm was assumed. Actually a standard objective with focal length f* hast to be chosen, that leads to a different field of view G* according to the objective’s reconstruction scale. V* = B f* = . G* g − f * What is an appropriate objective for the upper example? additionally given values: g = 200mm (defined by setup) B = 6.4mm (1/2” camera with sensor resolution of 1280x960px²) seeked values: f, f* (focal length) s* (measuring security) f= g⋅B 200 ⋅ 6.4mm² = = 13.27 mm G '+ B 90mm + 6.4mm To ensure the object lying completely within the image, a focal length f*=12mm is chosen. Finally, one has to check whether the reached camera resolution is still sufficient to provide an accuracy of s=0.02mm. 05.05.2009 B g− f * 200 − 12 = B⋅ = 6.4 ⋅ = 100.26mm V* f* 12 n px 0.25 = 100.26 ⋅ = 0.0195mm s* = G * ⋅ 1280 Rcamera G* = Dr. Pierre Elbischger - Camera Systems - MIP1/ISAP'SS09 30 Quantization The upper left image has 256 gray levels. In the following images the quantization resolution is halved. 05.05.2009 Dr. Pierre Elbischger - Camera Systems - MIP1/ISAP'SS09 31 Literature [1] Azad, P., and Gockel, T., and Dillmann, R. (2007): Computer Vision – Das Praxisbuch. [2] Sonka, M., and Hlavac, V., and Boyle, R. (2008): Image Processing, Analysis, and Machine Vision. 05.05.2009 Dr. Pierre Elbischger - Camera Systems - MIP1/ISAP'SS09 32 ...
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This note was uploaded on 07/09/2009 for the course MEDIT 1 taught by Professor Pierreelschbinger during the Spring '09 term at Carinthia University of Applied Sciences.

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