| | The GSMT Book: Chapter 4, Section 4.7.6.1 (Site not responding. Last check: 2007-10-26) |
 | | AO support high dynamic range imaging by improving the concentration of flux for an unresolved faint source (proportional to S, the Strehl ratio), and by reducing the amplitude of the noncoherent seeing halo (proportional to (1-S)). |
 | | In high dynamic range imaging (HDRI) applications, employing coronagraphy or nulling to suppress the coherent diffraction core results in the detection of the faintest sources usually being limited by speckle structure in the image, rather than by the photon noise. |
 | | High dynamic range imagery of bright sources will often be limited by speckle structure in the uncorrected halo of the bright source rather than by its photon noise, particularly if coronagraphy or nulling is employed to reduce the amplitude of the diffracted component. |
| www.aura-nio.noao.edu /book/ch4/4_7_6_1.html (4299 words) |