Imaging with a Coherence Interferometer in Optical Astronomy

Autor: C. Roddier, F. Roddier
Rok vydání: 1979
Zdroj: International Astronomical Union Colloquium. 49:175-185
ISSN: 0252-9211
Popis: In optical astronomy, images are highly degraded by atmospheric turbulence. The diameter of the seeing disk may vary from 0.2 arcseconds to 10 arcseconds or more according to weather conditions. A typical diameter is of the order of 2 arcseconds which is the angular resolution of a 6cm lens at the diffraction limit.Large telescopes have been built for their light collecting capabilities, not for their resolving power which is, in general, of the order of 0.2 arcseconds, that is far from the diffraction limit.
Databáze: OpenAIRE