Analysis of the observed r.m.s contrast in solar granulation

Details Analysis of the observed r.m.s contrast in solar granulation Analysis of the observed r.m.s contrast in solar granulation

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001acasn..42..134r&link_type=abstract

Acta Astronomica Sinica, vol.42, no.2, p. 134-139.

Astronomy and Astrophysics

Astronomy

1

Solar Granulation, R.M.S. Contrast, Atmospheric Coherent Length, Optical Transfer Function

Scientific paper

On the focal plane of the telescope and the detector, the relationships between the r.m.s. contrast in the solar granulation and the diameter of the telescope, the atmospheric coherent length and the detecting sensitivity of the system are analyzed respectively. The numerical results of the r.m.s. contrast in the solar granulation as functions of the diameter, the atmospheric coherent length and the detecting sensitivity of the system are presented. Furthermore, the related experimental results are given.

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