Speckle Observation of Binary Stars at NTNU
碩士 === 國立臺灣師範大學 === 地球科學系 === 97 === The binary image will be distorted by atmospheric turbulence, however the angular separation of a binary could be determined with speckle interferometry technology. The binary program with speckle interferometry at NTNU has been set up since 2002. The commercial...
| Main Authors: | , |
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| Other Authors: | |
| Format: | Others |
| Language: | en_US |
| Published: |
2009
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| Online Access: | http://ndltd.ncl.edu.tw/handle/18502550347649716756 |