Articles | Volume 3, issue 2
https://doi.org/10.5194/gi-3-241-2014
https://doi.org/10.5194/gi-3-241-2014
Research article
 | 
10 Dec 2014
Research article |  | 10 Dec 2014

Auroral all-sky camera calibration

F. Sigernes, S. E. Holmen, D. Biles, H. Bjørklund, X. Chen, M. Dyrland, D. A. Lorentzen, L. Baddeley, T. Trondsen, U. Brändström, E. Trondsen, B. Lybekk, J. Moen, S. Chernouss, and C. S. Deehr

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Cited articles

Akasofu, S. I.: The latitudinal shift of the auroral belt, J. Atmosph. Terr. Phys., 26, 1167–1174, 1964.
Gaertner, A.: Spectral radiance of low brightness source serial number 10113, Calibration report no. PAR-2012-3049, Institute for National Measurement Standards, National Research Council Canada, 1–11, 2013
Hunten, D. M., Roach, F. E., and Chamberlain, J. W.: A photometric unit for the airglow and aurora, J. Atmosph. Terr. Phys., 8, 345–346, 1956.
Kumler, J. J. and Bauer, M. L.: Fish-eye lens design and their relative performance, Proc. SPIE 4093, Current Developments in Lens Design and Optical Systems Engineering, 360 (24 October 2000), https://doi.org/10.1117/12.405226, 2000.
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Short summary
A two-step procedure to calibrate the spectral sensitivity of auroral all-sky (fish-eye) cameras is outlined. First, center pixel response is obtained by the use of a Lambertian surface and a standard tungsten lamp. Second, all-sky flat-field correction is carried out with an integrating sphere.