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More about some of WinSCANOPY's features
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The WinSCANOPY Pro DSLR Version
DSLR stands for Digital Single Lens Reflex cameras. These cameras are high-end digital (filmless) models that are based on and operate like professional 35mm film cameras. DSLR camera lenses are fully interchangeable, they dont have a non removable lens like point-and-shoot cameras. They accept standard high quality lenses made for 35mm film cameras or newer lenses made especially for them. Our DSLR cameras are completely automatic (the camera sets the proper exposure and aperture) but all of them allow complete manual control over all camera settings. The typical resolution of images produced by DSLR cameras is in the range of 10 to 20 megapixels (subject to change). The images they produce have an outstanding clarity and definition.
The WinSCANOPY Pro DSLR version has its default settings configured for DSLR cameras images which have a different aspect ratio than Point and Shoot cameras. It can also analyse images with 10 to 16 bits of grey levels information produced by such high end cameras and it can extract GPS information from camera image files when a GPS unit is connected to the camera (only some models support this feature and GPS units are not sold by Regent Instruments).
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Multiple Passes Analysis (Pro DSLR version)
To analyse images more than one time with different parameters in a single mouse click
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| WinSCANOPY can process images in multiple passes by successively analyzing them under a different set of parameters (sky grids, lens FOV...) for each pass. Some applications can be: 1) to obtain the same sky divisions as another research project for comparison purposes, while at the same time analyzing the image under optimal (or other standard) divisions and 2) to analyse gap fractions at different overlaping zenith ranges [Ex: 0-10º, 0-20º, 10-60º...]. |
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WinSCANOPY has five (Reg) or six (Pro) methods of calculating LAI. Most of them are available in two variations; the linear and the log average (the latter is for foliage clumping compensation with the Lang and Xiang 86 method).
- Bonhomme and Chartier: This method is based on the assumption that at 57.5 degrees of elevation (user changeable), gap fraction is insensitive to leaf angle and can be related to LAI by the Beer-Lambert extinction law.
LAI-2000 original: The method is based on the work of Miller (1967) and Welles and Norman (1991). It uses linear regression to relate LAI to gap fractions at different zenith angles. It can also be used to measure isolated tree leaf density by substituting the default path lengths (valid for a continuous canopy) to those of the tree.
- LAI-2000 generalized: This method is similar to the LAI-2000 original method. The formulae used for calculations originate from the same theory but have been generalized for any number of elevation rings and field of view.
- Spherical: This method assumes that leaf area distribution in canopies is identical to that of a sphere.
- Ellipsoid: This method (Campbell, 1985) assumes that leaf area distribution in canopies is similar to that of an ellipsoid and uses non-linear curve fitting to relate LAI to gap fractions.
- 2D projected area: method to measure individual tree leaf area is the area meter method first described by Lindsey and Bassuk 1992 and later modified and tested by Peper and McPherson 1998. We have enhanced the method so that calibration is much easier than described by the authors.
- Bonhomme R. & Chartier P. 1972. The Interpretation and Automatic Measurement of Hemispherical Photographs to Obtain Sunlit Foliage Area and Gap Frequency. Israel Journal of Agricultural Research 22. pp. 53-61.
- Miller J.B. 1967, A formula For Average Foliage Density. Aust. J. Bot. 15, pp. 141-144.
- Welles J. M. and Norman J. M. 1991, Instrument for Indirect Measurement of Canopy Architecture, Agronomy Journal 83, pp. 818-825.
- Campbell G.S., 1985. Extinction Coefficients for Radiation in Plant Canopies Calculated Using an Ellipsoidal Inclination Angle Distribution. Agric. For. Meteorol., 36, pp. 317-321.
- Lang A.R.G., Xiang Y.Q., 1986, Estimation of leaf area index from transmission of direct sunlight in discontinuous canopies. Agric. For. Meteor. 37: pp. 229-243.
- Lindsey P.A. and Bassuk N. L., 1992. A nondestructive image analysis technique for estimating whole-tree leaf area. HortTechnology, 2 (1) pp. 66-72.
- Peper P. J. and McPherson E. G., 1998. Comparison of five methods for estimating leaf area index of open grown deciduous trees. Journal of Arboriculture, 24 (2), pp. 98-111.
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Pixels classification
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| An accurate classification of pixels into the sky (gaps) and canopy categories is a pre-requisite to get precise canopy analyses from hemispherical images. WinSCANOPY offers different methods to do this classification and to modify it after if required.
All WinSCANOPY versions have a global automatic threshold method which has been improved in 2006. This method uses grey levels information (light intensity from a color or grey levels image) to decide in which class (sky or canopy) pixels belongs to. With a global threshold, the classification criteria is the same for all pixels of the hemisphere.
The Pro DSLR version offers four additional methods to classify pixels, two of which are specific to hemispherical images.
- An adaptive threshold that changes value in function of the location in the hemisphere. It adapts itself in function of the lighting variations.
- An hemispherical threshold that takes into account the light variation of hemispherical lenses which are brighter at the zenith and darker at the horizon.
- A threshold that takes into account the light variations due to the sun position in the image (indicated by the operator). The attenuation compensation can be linear or like the SOC diffuse radiation distribution.
- Classification based on true color. This algorithm is more tolerant to sky conditions variations. For example, it allows to analyse images with white clouds and dark blue sky, a task difficult to do with simple grey levels thresholds (the dark blue sky tend to be classified as canopy).
The result of the pixels classification can be viewed before the analysis or after. As you change the parameters, the resulting classification is shown in the displayed image allowing you to choose the best method.
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The pixels classification can be verified and modified for specific image regions at any moment of the analysis. Pixels that fall into the canopy group are drawn a different color over the original image as the threshold (pixel classification criteria) is modified by moving a slider bar. This allows for a simultaneous view of the original and pixels classification images.
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Select a region to be classified. It can be the whole image, a sub-region of any shape defined by outlining it or a pre-defined circular regions corresponding to the sky grid's zenith rings or circular regions centered on the sky brightest position (below).
As you move the slider, pixels classified into the canopy groups are drawn in green over the original image.
Adjust the slider so that all canopy elements are covered by green pixels (but not the sky). The analysis is updated automatically.
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The image to the left has a non-uniform sky light distribution. It is well analysed with our solar threshold which adjusts its strength in function of position in the hemisphere. In this case, a global threshold or a threshold adjusted in function of the sky grid (centered on the zenith) is not efficient. |
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Color analysis is more tolerant to sky condition variations.
Images with clouds and blue sky or blue sky alone can often be analyzed.
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The left side image is more easily analysed in color than in grey levels due to the presence of dark blue sky which tends to be classified as canopy in a grey levels analysis.
White stems (right image) are often misclassified as sky with a threshold based method. With color classification this is not a problem (when no white clouds are present)
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10 to 16 bits of grey levels per pixels images (like those produced by DSLR cameras) offers new pixels classification opportunities.
An image with more bits per pixel has a wider dynamic range (difference between darkest and brightest light levels) and more tonal variations (smallest light variations that can be distinguished). When the number of grey levels is not sufficient, light variations are merged into the same grey level information is lost. When subtle light variations are preserved, this gives more choices for pixels classification into canopy and sky
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Masks
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| It is possible to mask some areas of the image to prevent them from being analysed. These regions might contain non-canopy elements like an operator, a building or a light that indicates the north direction. There can be as many as you wish, they can have any shape and can be created by different methods (see below). Unlike their hardware counter part, they can be added and modified after the image has been taken. You can export and import masks (even from other programs) to files (unlimited number of masks per file), save them with the image (in the same tiff file) and revert a masked region (the masked area can be the inside or outside of the mask). |
There are four types of masks and two variations of them;
- Interactive masks are created simply by drawing in the image with a lasso tool. The masked area can be inside or outside the outlined area.
- Parametrical masks are created by specifying geometrical parameters tied to the hemisphere position and size in the image. These parameters comprise the azimuth and elevation beginning and ending angles and how they vary in between.
- Coordinate masks are defined by entering a series of hemisphere coordinate points (azimuth and elevation or zenith).
- Image masks are created by loading an image and transforming it to a mask before an analysis.
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| 1) Interactive masks. They are made by drawing in the image. They usually have an irregular shape. |
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Inside masks. The masked area is the interior of the region outlined by the operator. |
Outside mask. The masked area is the exterior of the region outlined by the operator. |
| 2) Parametrical masks. They are made by specifying hemispherical parameters. They usually have a regular shape. |
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| 3) Coordinates masks. They are made by specifying image or hemispherical point coordinates. They can have any shape. |
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| 4) An image mask is an image stored in a tiff or jpeg file which indicates areas of the image to be masked (not analysed). They can be produced by many types of programs (image editors, GIS programs which compute view sheds based on digital elevation models,...) or within WinSCANOPY itself by drawing the mask with the edition tools. |
Individual Gaps Measurement |
| The position, size (area), gap fraction and radiation data of canopy gaps can be measured by outlining them in the image. See also the automatic gaps size distribution analysis |
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WinSCANOPY 2006a
Measurements & Features |
Gap Size Distribution Analysis (Pro DSLR) - (new since 2006a)
Gap size distribution (GSD), i.e. the number of gaps in function of their size, can be used in combination with gap fractions to quantify the degree of clumpiness at the tree level and to use this information to increase the accuracy of LAI measurements. For a canopy of a given gap fraction with randomly distributed foliage elements, it is possible to make a theoretical probability of gaps occurring in function of their size. By comparing the measured GSD to this theoretical distribution, foliage clumpiness can be measured.
At the base of GSD analysis, is the classification of gaps in two categories; those which are normally expected for a given randomly distributed leaf area and those which are not. The latter are larger gaps that are present because of foliage clumping at the crown level and can be seen between tree crowns. These are called between-crown gaps while random gaps are called within-crown gaps. WinSCANOPY has two methods of classifying gaps into these two groups; Chen and Cihlar 95's method based on transect length (a one dimensional data), which is also used in a sunfleck based commercial instrument, and a new simpler, but efficient, method of our own based on gap area (a two dimensional data).
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GSD analyses can be done on hemispherical or cover images. Between-crown gaps are drawn in blue,
within-crown gaps are drawn in yellow. |
Other features of GSD
> On-screen visualisation of between-crown and within-crown gaps. Can also be saved to standard tiff image files.
> The automatic gap classification can be modified with simple mouse clicks. It can also be done completely manually.
> Clumping index is measured in function of view zenith angle and globally for the hemisphere or for any view angles range that you choose. Clumping index in function of zenith can be displayed in the graphic above the image during the analysis. |
Highest obstruction per azimuth analysis (Basic) - (new since 2006a)
It gives the zenith angle of the highest obstacle (canopy, building or any object other than sky) in function of azimuth. Useful for shading analysis (solar panels, architecture) and communication equipment site comparisons.
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References
- Chen J.M. and Cihlar J., 1995, Plant canopy gap-size analysis theory for improving optical measurements of leaf-area index, Applied Optics Vol. 34. no. 27, pp. 6211-6222
- Lindsey P.A. and Bassuk N. L., 1992. A nondestructive image analysis technique for estimating whole-tree leaf area. HortTechnology, 2 (1) pp. 66-72
- Peper P. J. and McPherson E. G., 1998. Comparison of five methods for estimating leaf area index of open grown deciduous trees. Journal of Arboriculture, 24 (2), pp. 98-111
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