Zobrazeno 1 - 10
of 17
pro vyhledávání: '"R. Q. Fugate"'
Autor:
R. Q. Fugate
Publikováno v:
SPIE Proceedings.
This paper discusses the concept of employing artificial guide stars to correct atmospheric turbulence induced wavefront distortion for Extremely Large Telescopes (ELTs) conducting science observations at near IR and visible wavelengths. A set of gen
Autor:
R. Q. Fugate
Publikováno v:
Symposium - International Astronomical Union. 158:293-295
The Starfire Optical Range 1.5 m telescope is equipped with a 241 actuator adpative optics system operating at visible wavelengths. The system can use either natural or laser guide star beacons for sensing wavefront distortions induced by atmospheric
A prototype cross-dispersed optical echelle spectrograph of very high resolution has been designed and built at Steward Observatory and tested at the Starfire Optical Range (SOR) 1.5 m telescope. It is the first spectrograph to take advantage of diff
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b8e664f6e20e3733fbf14f264f3fffe3
Autor:
P. H. Roberts, David L. Fried, R. E. Ruane, B. R. Boeke, Glenn A. Tyler, Guillermo A. Ameer, R. Q. Fugate, L. M. Wopat, S. L. Browne
Publikováno v:
Nature. 353:144-146
THE possibility of using an artificial 'guide-star' to measure optical wavefront distortion caused by atmospheric turbulence has been discussed for some time1–4, but few experimental data are available5. Here we report experimental results demonstr
Publikováno v:
Nature. 351:300-302
ANGEL et al.1 recently showed how an artificial neural network could be used to measure optical phase distortion induced by atmospheric turbulence, and demonstrated by numerical simulation that such a system could be used to control the six 1.8-m mir
Autor:
R. Q. Fugate
Publikováno v:
Pulsed Metal Vapour Lasers ISBN: 9789401072472
This paper discusses the use of copper-vapor lasers as sources of artificial guide stars for ground-based telescope adaptive-optics systems. In particular, the system in use at the 1.5-m telescope at the USAF Phillips Laboratory Starfire Optical Rang
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::74edc8c1f5369700075b1b6aa0a3b824
https://doi.org/10.1007/978-94-009-1669-2_46
https://doi.org/10.1007/978-94-009-1669-2_46
Autor:
J. Ge, B. Jacobsen, J.R.P. Angel, N. Woolfv, J. H. Black, M. Lloyd-Hart, P. Gray, R. Q. Fugate
Publikováno v:
Adaptive Optics.
A prototype optical wavelength ultrahigh resolution echelle cross-dispersed spectrograph has been tested at the Starfire Optical Range (SOR) 1.5 m telescope (Woolf et al. 1995; Ge et al. 1996). To our knowledge this is the first high resolution spect
Publikováno v:
Signal Recovery and Synthesis.
The release of military technology in the adaptive optics (AO) and laser beacons fields [1] motivated the astronomical community to become actively involved in its implementation in astronomical sites all around the world. Unfortunately, even with th
Autor:
R. Q. Fugate
Publikováno v:
Very High Angular Resolution Imaging ISBN: 9780792326335
The Starfire Optical Range 1.5 rn telescope is equipped with a 241 actuator adpative optics system operating at visible wavelengths. The system can use either natural or laser guide star beacons for sensing wavefront distortions induced by atmospheri
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f3d34e337165e7dd3a08b15a78c6ec19
https://doi.org/10.1007/978-94-011-0880-5_49
https://doi.org/10.1007/978-94-011-0880-5_49
Autor:
T. K. Barrett, D. G. Sandler, R. Q. Fugate, B. A. Ellerbroek, M. T. Donovan, C. H. Higgins, J. M. Spinhirne
Publikováno v:
Adaptive Optics for Large Telescopes.
Simulations and earlier off-line experimental data suggest1,2 that a wavefront sensor based on an artificial neural network processor may provide a simple way to measure low-order wavefront distortion in an astronomical telescope. The neural network