This repository contains code for processing all-sky images generated by the Mid-latitude All-sky-imager Network for Geophysical Observations (MANGO), a project funded by the National Science Foundation.
Currently, mosaic images are found by interpolating raw image files to a common, regular geodetic latitude/longitude grid. This is slow, and can create some distortion effects because the grid is not evenly spaced. Investigate ways of improving this algorithm.
Don't interpolate at all, use the original positions and find another way to determine camera hiarchy in the mosaic image
Make the grid easily adaptable instead of hard-coded
Currently, mosaic images are found by interpolating raw image files to a common, regular geodetic latitude/longitude grid. This is slow, and can create some distortion effects because the grid is not evenly spaced. Investigate ways of improving this algorithm.