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In astronomy, seeing is the degradation of the image of an astronomical object due to turbulence in the atmosphere of Earth that may become visible as blurring, twinkling or variable distortion. The origin of this effect is rapidly changing variations of the optical refractive index along the light path from the object to the detector. Seeing is a major…
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seeing telescope turbulence astronomical displaystyle atmosphere diameter image telescopes resolution r0 parameter optical atmospheric right fried mathbf left phase fluctuations
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| Mars | instance of | In viewing a bright object | 0.80 | text |
| occasionally a still patch of air will come in front of the planet | instance of | In viewing a bright object | 0.80 | text |
| resulting in a brief moment of clarity | instance of | In viewing a bright object | 0.80 | text |
| the Navy Prototype Optical Interferometer or Cambridge Optical Aperture Synthesis Telescope | instance of | The highest resolution visible and infrared images currently come from imaging optical interferometers | 0.80 | text |
| but those can only be used on very bright stars.Starting in the 1990s | instance of | The highest resolution visible and infrared images currently come from imaging optical interferometers | 0.80 | text |
| many telescopes have developed adaptive optics systems that partially solve the seeing problem | instance of | The highest resolution visible and infrared images currently come from imaging optical interferometers | 0.80 | text |
| Astronomical seeing | has effect | Astronomical | 0.60 | section |
| Astronomical seeing | has effect | It | 0.60 | section |
| Astronomical seeing | has effect | Airy | 0.60 | section |
| Astronomical seeing | has effect | Long | 0.60 | section |
| Astronomical seeing | has effect | CN2 | 0.60 | section |
| Astronomical seeing | related to Measures | There | 0.60 | section |
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