My artwork is fortified by three essential elements, vibrant color, luminous light, and repeated patterns found in nature. These elements unify my oil paintings and computer generated artwork and form a substructure that serves to magnify the unique concord found in nature.

I have created art that has evolved from my own personal experiences. Life is capricious, and with the changes wrought by age, joy, and grief, I have found this self-referential work inevitable. Here, I have documented the journey that has brought me through personal wars, battles, and truces. I have come to believe that although my individual experiences may be unique, my responses to them are not. Loss and victory are universal.

<p><font face="Arial"> <p align="left">The aim of this study is to compare proximal caries depth on unenhanced storage phosphor plate images and conventional film images. The phosphor plate images were then copied by increasing and decreasing both contrast and brightness respectively. The enhanced phosphor plate images were compared with the unenhanced storage phosphor plate images and conventional film images for the detection of proximal caries diagnosis.</p> </font></p>

<p><font face="Arial"> <p align="left">The aim of this study is to compare proximal caries depth on unenhanced storage phosphor plate images and conventional film images. The phosphor plate images were then copied by increasing and decreasing both contrast and brightness respectively. The enhanced phosphor plate images were compared with the unenhanced storage phosphor plate images and conventional film images for the detection of proximal caries diagnosis.</p> </font></p>

Yes / PICARD is a space-based observatory hosting the Solar Diameter Imager and Surface Mapper (SODISM) telescope, which has continuously observed the Sun from July 2010 and up to March 2014. In order to study the fine structure of the solar surface, it is helpful to apply techniques that enhance the images so as to improve the visibility of solar features such as sunspots or faculae. The objective of this work is to develop an innovative technique to enhance the quality of the SODISM images in the five wavelengths monitored by the telescope at 215.0 nm, 393.37 nm, 535.7 nm, 607.1 nm and 782.2 nm. An enhancement technique using interpolation of the high-frequency sub-bands obtained by Discrete Wavelet Transforms (DWT) and the input image is applied to the SODISM images. The input images are decomposed by the DWT as well as Stationary Wavelet Transform (SWT) into four separate sub-bands in horizontal and vertical directions namely, low-low (LL), low-high (LH), high-low (HL) and high–high (HH) frequencies. The DWT high frequency sub-bands are interpolated by a factor 2. The estimated high frequency sub-bands (edges) are enhanced by introducing an intermediate stage using a stationary Wavelet Transform (SWT), and then all these sub-bands and input image are combined and interpolated with half of the interpolation factor α/2, used to interpolate the high-frequency sub-bands, in order to reach the required size for IDWT processing. Quantitative and visual results show the superiority of the proposed technique over a bicubic image resolution enhancement technique. In addition, filling factors for sunspots are calculated from SODISM images and results are presented in this work.