会议论文详细信息
| Adapting to the Atmosphere Conference 2014 | |
| Characterising atmospheric optical turbulence using stereo-SCIDAR | |
| 物理学;地球科学 | |
| Osborn, James^1 ; Butterley, Tim^1 ; Föhring, Dora^1 ; Wilson, Richard^1 | |
| Department of Physics, Centre for Advanced Instrumentation, University of Durham, South Road, Durham | |
| DH1 3LE, United Kingdom^1 | |
| 关键词: Isaac newton telescope; Optical turbulence; Scintillation detection; | |
| Others : https://iopscience.iop.org/article/10.1088/1742-6596/595/1/012022/pdf DOI : 10.1088/1742-6596/595/1/012022 |
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| 来源: IOP | |
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【 摘 要 】
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.
【 预 览 】
| Files | Size | Format | View |
|---|---|---|---|
| Characterising atmospheric optical turbulence using stereo-SCIDAR | 861KB |
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