However, the geometric normalization of the preprocessing phase subsequently uses eye location to scale the probes (and the gallery images) to have consistent eye locations and overall face dimensions of a 130-pixel width and a 150-pixel height, regardless of input image size or optical resolution.
We used the wave height for a return period of 50 years and set the height of the input wave to 13.1 m.
We employed the wave height for the 50-year return period and set the height of the input wave to 13.1 m.
where w and h are the width and height of the input image in pixels, respectively; I R, I G, I B are the R, G and B components in the RGB colour space, respectively; and I RG and I BG are the R/G and B/G components in the representation of the image in (R/G, B/G) space.
for x=0...w,y=0...h, where w and h are the width and height of the input image in pixels, respectively; I RG and I BG are the R/G and B/G components in the representation of the image in (R/G, B/G) space, respectively; I is the searched area; and T 1 and T 2 are the threshold values.
Consequently, RiskScape also uses a HEMU of height in metres, input as raster or a single polygon denoting edifice extent.
Remarks: 1) Using observed plume heights of 2.9 3.3 km as input parameter, 2) using a windspeed of 20 m/s at 500 hPa (~5.2 km height) as input parameter, 3) cylindrical conduit with a diameter of 50 m was assumed, and 4) source diameter of 6 m was assumed, 40 75 % of total diameter according to Dürig et al. (2015); see text for details.
The topside scale height (Ts) and transition height (Th) models, previously developed by the authors, provided Ts and Th for any set of input parameters: month, local time, geomagnetic latitude, solar flux F107, and Kp.
You'll find the width (W) and height (H) input fields in the bottom left part of the aforementioned panel.
