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A two-step procedure to calibrate the spectral sensitivity to visible light of auroral all-sky cameras is outlined. Center pixel response is obtained by the use of a Lambertian surface and a
Published by: Geoscientific Instrumentation, Methods and Data Systems Published on:
YEAR: 2014   DOI: 10.5194/gi-3-241-2014
Published by: Comptes rendus de l’Acad\ emie bulgare des Sciences Published on: