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Characterising atmospheric optical turbulence using stereo-SCIDAR

Journal of Physics: Conference Series (2015) 595(1)
DOI: 10.1088/1742-6596/595/1/012022
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Abstract

Stereo-SCIDAR (SCIntillation Detection and Ranging) is a development to the well known SCIDAR method for characterisation of the Earth's atmospheric optical turbulence. Here we present some interesting capabilities, comparisons and results from a recent campaign on the 2.5 m Isaac Newton Telescope on La Palma.

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Osborn, J., Butterley, T., Föhring, D., & Wilson, R. (2015). Characterising atmospheric optical turbulence using stereo-SCIDAR. In Journal of Physics: Conference Series (Vol. 595). Institute of Physics Publishing. https://doi.org/10.1088/1742-6596/595/1/012022

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