Multi-star Turbulence Monitor: A new technique to measure optical turbulence profiles

10 Oct 2019 Hickson Paul Ma Bin Shang Zhaohui Xue Suijian

The strength and vertical distribution of atmospheric turbulence is a key factor determining the performance of optical and infrared telescopes, with and without adaptive optics. Yet, this remains challenging to measure... (read more)

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  • INSTRUMENTATION AND METHODS FOR ASTROPHYSICS