Abstract:Light microscopy enlarges the viewing angle while decreasing the depth of focus. This leads to mainly blurred images if the specimen being observed consists of significant high changes. In computer vision solving this problem is known as 'shape from focus'. Algorithms exist that perform both, the calculation of a sharp image and the recovery of the three dimensional structure of the specimen. In this paper three classic approaches for detecting sharp image regoins are evaluated. Three new so called focus measu… Show more
“…One of the methods with a very impressive performance is Helmli and Scherer's mean method (MIS5), proposed by Helmli and Scherer (2001). This technique provided very good results for the whole range of D/r 0 conditions and both types of observed solar regions.…”
Section: Resultsmentioning
confidence: 99%
“…It is noteworthy that, the original idea had to be slightly modified to enhance the method performance. On the other hand, when the seeing conditions cover a wide range, the most efficient method is Helmli and Scherer's mean (Helmli and Scherer, 2001), (MIS5). This method should be considered when observing without AO or when the seeing conditions are unknown.…”
Observations of the solar photosphere from the ground encounter significant problems caused by Earth's turbulent atmosphere. Before image reconstruction techniques can be applied, the frames obtained in the most favorable atmospheric conditions (the socalled lucky frames) have to be carefully selected. However, estimating the quality of images containing complex photospheric structures is not a trivial task, and the standard routines applied in nighttime lucky imaging observations are not applicable. In this paper we evaluate 36 methods dedicated to the assessment of image quality, which were presented in the literature over the past 40 years. We compare their effectiveness on simulated solar observations of both active regions and granulation patches, using reference data obtained by the Solar Optical Telescope on the Hinode satellite. To create images that are affected by a known degree of atmospheric degradation, we employed the random wave vector method, which faithfully models all the seeing characteristics. The results provide useful information about the method performances, depending on the average seeing conditions expressed by the ratio of the telescope's aperture to the Fried parameter, D/r 0 . The comparison identifies three methods for consideration by observers: Helmli and Scherer's mean, the median filter gradient similarity, and the discrete cosine transform energy ratio. While the first method requires less computational effort and can be used effectively in virtually any atmospheric conditions, the second method shows its superiority at good seeing (D/r 0 < 4). The third method should mainly be considered for the post-processing of strongly blurred images.
“…One of the methods with a very impressive performance is Helmli and Scherer's mean method (MIS5), proposed by Helmli and Scherer (2001). This technique provided very good results for the whole range of D/r 0 conditions and both types of observed solar regions.…”
Section: Resultsmentioning
confidence: 99%
“…It is noteworthy that, the original idea had to be slightly modified to enhance the method performance. On the other hand, when the seeing conditions cover a wide range, the most efficient method is Helmli and Scherer's mean (Helmli and Scherer, 2001), (MIS5). This method should be considered when observing without AO or when the seeing conditions are unknown.…”
Observations of the solar photosphere from the ground encounter significant problems caused by Earth's turbulent atmosphere. Before image reconstruction techniques can be applied, the frames obtained in the most favorable atmospheric conditions (the socalled lucky frames) have to be carefully selected. However, estimating the quality of images containing complex photospheric structures is not a trivial task, and the standard routines applied in nighttime lucky imaging observations are not applicable. In this paper we evaluate 36 methods dedicated to the assessment of image quality, which were presented in the literature over the past 40 years. We compare their effectiveness on simulated solar observations of both active regions and granulation patches, using reference data obtained by the Solar Optical Telescope on the Hinode satellite. To create images that are affected by a known degree of atmospheric degradation, we employed the random wave vector method, which faithfully models all the seeing characteristics. The results provide useful information about the method performances, depending on the average seeing conditions expressed by the ratio of the telescope's aperture to the Fried parameter, D/r 0 . The comparison identifies three methods for consideration by observers: Helmli and Scherer's mean, the median filter gradient similarity, and the discrete cosine transform energy ratio. While the first method requires less computational effort and can be used effectively in virtually any atmospheric conditions, the second method shows its superiority at good seeing (D/r 0 < 4). The third method should mainly be considered for the post-processing of strongly blurred images.
“…A subsequent approach (referred to as Focused Image Surface) locally tries to refine the initial recovered topography D by optimizing both position and orientation of 2-D planar (then curved) windows throughout the 3-D measure F so as to maximize the covered degrees of focus (Ahmad & Choi, 2005;Asif & Choi, 2001;Subbarao & Choi, 1995;Yun & Choi, 1999). Finally, the topography is often smoothed through average, median or recently bilateral filters (Helmli & Scherer, 2001;Khan et al, 2010;Niederöst et al, 2003). Interpolation techniques lying beyond the scope of this paper, only the traditional one will be used herein, sometimes finalised by a median filter.…”
“…This defocusing measurement is mainly done with Laplacian operators, which computes the second spatial derivative for every point in a neighbourhood of N pixels in each direction. Many other operators have been proposed, and a review of them can be found in (Helmi & Scherer, 2001). …”
scite is a Brooklyn-based organization that helps researchers better discover and understand research articles through Smart Citations–citations that display the context of the citation and describe whether the article provides supporting or contrasting evidence. scite is used by students and researchers from around the world and is funded in part by the National Science Foundation and the National Institute on Drug Abuse of the National Institutes of Health.