Wavefront outer scale deduced from interferometric dispersed fringes
暂无分享,去创建一个
Julien Borgnino | Aziz Ziad | D. Mourard | F. Patru | François Martin | Daniel Bonneau | S. Jankov | J. Maire
[1] M. Shao,et al. Atmospheric phase measurements with the Mark III stellar interferometer. , 1987, Applied optics.
[2] F. Roddier,et al. Interferometric imaging in optical astronomy , 1988 .
[3] C. Aime,et al. Polychromatic transfer functions in stellar speckle interferometry , 1989 .
[4] Julien Borgnino,et al. Comparison of measurements of the outer scale of turbulence by three different techniques. , 2004, Applied optics.
[5] F Roddier,et al. Long-baseline Michelson interferometry with large ground-based telescopes operating at optical wavelengths. I. General formalism. Interferometry at visible wavelengths , 1984 .
[6] Keh-Shew Lu,et al. DIGITAL FILTER DESIGN , 1973 .
[7] R Conan,et al. From the grating scale monitor to the generalized seeing monitor. , 2000, Applied optics.
[8] A. Blazit,et al. Dispersed fringe tracking with the multi-r(0) apertures of the Grand Interféromètre à 2 Télescopes. , 1996, Applied optics.
[9] Christopher A. Haniff,et al. Atmospheric phase fluctuation measurement: interferometric results from the WHT and COAST telescopes , 1994, Astronomical Telescopes and Instrumentation.
[10] Julien Borgnino,et al. EFFECTS OF ATMOSPHERIC SPECTRAL DECORRELATION ON VISIBILITY MEASUREMENTS IN MICHELSON INTERFEROMETRY , 1997 .
[11] D. Buscher,et al. Interferometric seeing measurements at the La Palma Observatory , 1991 .
[12] Denis Mourard,et al. Removing the photon-centroiding hole in optical stellar interferometry , 1998 .
[13] David Le Mignant,et al. Atmospheric turbulence characterization with the Keck adaptive optics systems. I. Open-loop data. , 2003, Applied optics.
[14] A. Agabi,et al. Optical parameters relevant for High Angular Resolution at Paranal from GSM instrument and surface layer contribution , 2000 .
[15] Influence of exposure time on spectral properties of turbulence-degraded astronomical images , 1975 .
[16] William C. Danchi,et al. Atmospheric Fluctuations: Empirical Structure Functions and Projected Performance of Future Instruments , 1992 .
[17] M. M. Colavita,et al. Atmospheric Turbulence Measurements with the Palomar Testbed Interferometer , 2001, astro-ph/0102052.
[18] C. Aime. Teaching astronomical speckle techniques , 2001 .
[19] Julien Borgnino,et al. Theoretical spatiotemporal analysis of angle of arrival induced by atmospheric turbulence as observed with the grating scale monitor experiment , 1997 .
[20] Julien Borgnino,et al. Effect of a finite spatial-coherence outer scale on the covariances of angle-of-arrival fluctuations , 1992 .
[21] John Davis,et al. Atmospheric path variations for baselines up to 80m measured with the Sydney University Stellar Interferometer , 1995 .
[22] M. M. Colavita,et al. Interferometric seeing measurements on Mt. Wilson: power spectra and outer scales. , 1995, Applied optics.
[23] Measurements of Stellar Speckle Interferometry Lens-atmosphere Modulation Transfer Function , 1979 .
[24] J. Mariotti,et al. Pathlength stability of synthetic aperture telescopes - The case of the 25 CM CERGA interferometer , 1984 .
[25] Thierry Fusco,et al. NAOS on-line characterization of turbulence parameters and adaptive optics performance , 2004 .
[26] T. W. Parks,et al. Digital Filter Design , 1987 .
[27] B. Roy Frieden,et al. Probability, Statistical Optics, And Data Testing , 1982 .
[28] Aziz Ziad,et al. Measurements of the wavefront outer scale at Paranal: influence of this parameter in interferometry , 2000, Astronomical Telescopes and Instrumentation.