PROCEEDINGS VOLUME 4840
ASTRONOMICAL TELESCOPES AND INSTRUMENTATION | 22-28 AUGUST 2002
Future Giant Telescopes
IN THIS VOLUME

0 Sessions, 60 Papers, 0 Presentations
AO for FGTs  (4)
Conclusion  (1)
ASTRONOMICAL TELESCOPES AND INSTRUMENTATION
22-28 August 2002
Waikoloa, Hawai'i, United States
AO for FGTs
Proc. SPIE 4840, MCAO for ELTs, 0000 (30 January 2003); doi: 10.1117/12.459973
Proc. SPIE 4840, Multiconjugate adaptive optics for a new generation of giant telescopes, 0000 (30 January 2003); doi: 10.1117/12.458170
Proc. SPIE 4840, Multiple-resolution (and field of view) adaptive optics: for ELTs only, 0000 (30 January 2003); doi: 10.1117/12.458186
Proc. SPIE 4840, Adaptive optics for the Euro50: design and performance, 0000 (30 January 2003); doi: 10.1117/12.458028
Poster Session
Proc. SPIE 4840, Results of AO simulations for ELTs, 0000 (30 January 2003); doi: 10.1117/12.457998
Proc. SPIE 4840, Near-infrared AO coronagraph design for giant telescopes, 0000 (30 January 2003); doi: 10.1117/12.459874
Proc. SPIE 4840, Layer-oriented single- and dual-field-of-view performance for OWL, 0000 (30 January 2003); doi: 10.1117/12.458077
Proc. SPIE 4840, Control strategy for the adaptive optics of the Euro50, 0000 (30 January 2003); doi: 10.1117/12.458040
Proc. SPIE 4840, Noise-free detectors in the visible and infrared: implications for the design of next-generation AO systems and large telescopes, 0000 (30 January 2003); doi: 10.1117/12.457980
Proc. SPIE 4840, Atmospheric-induced wavefront distortion and compensation on large-aperture millimeter-wave telescopes, 0000 (30 January 2003); doi: 10.1117/12.457968
Proc. SPIE 4840, Reconstructing wavefronts with varying Hartmann arrays, 0000 (30 January 2003); doi: 10.1117/12.457967
Ongoing Designs I
Proc. SPIE 4840, Progress on the California Extremely Large Telescope (CELT), 0000 (30 January 2003); doi: 10.1117/12.464902
Proc. SPIE 4840, CELT optics alignment procedure, 0000 (30 January 2003); doi: 10.1117/12.459966
Proc. SPIE 4840, Control of the California Extremely Large Telescope primary mirror, 0000 (30 January 2003); doi: 10.1117/12.458150
Proc. SPIE 4840, Diffraction effects from giant segmented mirror telescopes, 0000 (30 January 2003); doi: 10.1117/12.457985
Proc. SPIE 4840, Large petal telescope for the next-generation Canada-France-Hawaii Telescope, 0000 (30 January 2003); doi: 10.1117/12.458071
Ongoing Designs II
Proc. SPIE 4840, Giant Segmented Mirror Telescope: a point design based on science drivers, 0000 (30 January 2003); doi: 10.1117/12.459863
Proc. SPIE 4840, Active optics and control architecture for a giant segmented mirror telescope, 0000 (30 January 2003); doi: 10.1117/12.459850
Proc. SPIE 4840, Modern control for the secondary mirror of a Giant Segmented Mirror Telescope, 0000 (30 January 2003); doi: 10.1117/12.458195
Proc. SPIE 4840, Diffraction in OWL: effects of segmentation and segments edge misfigure, 0000 (30 January 2003); doi: 10.1117/12.459957
Ongoing Designs III
Proc. SPIE 4840, 20- and 30-m telescope designs with potential for subsequent incorporation into a track-mounted pair (20/20 or 30/30), 0000 (30 January 2003); doi: 10.1117/12.459862
Proc. SPIE 4840, Optics for the 20/20 telescope, 0000 (30 January 2003); doi: 10.1117/12.459968
Proc. SPIE 4840, Mechanical concepts for 30-m class telescopes, 0000 (30 January 2003); doi: 10.1117/12.459860
Proc. SPIE 4840, The Euro50 extremely large telescope, 0000 (30 January 2003); doi: 10.1117/12.458049
Poster Session
Proc. SPIE 4840, OWL wind loading characterization: a preliminary study, 0000 (30 January 2003); doi: 10.1117/12.459981
Proc. SPIE 4840, Design and preliminary test of a precision segment positioning actuator for the California Extremely Large Telescope primary mirror, 0000 (30 January 2003); doi: 10.1117/12.459974
Proc. SPIE 4840, Giant Segmented Mirror Telescope (GSMT) structure: a conceptual design, 0000 (30 January 2003); doi: 10.1117/12.459958
Proc. SPIE 4840, Friction drive and bogies for OWL's main axes: technological step backwards or cost effective alternative, 0000 (30 January 2003); doi: 10.1117/12.459931
Proc. SPIE 4840, Site survey for the Giant Segmented Mirror Telescope, 0000 (30 January 2003); doi: 10.1117/12.459881
Proc. SPIE 4840, The SALT mirror mount: a high-performance low-cost mount for segmented mirrors, 0000 (30 January 2003); doi: 10.1117/12.459866
Proc. SPIE 4840, Design and analysis of 20-m track-mounted and 30-m telescopes, 0000 (30 January 2003); doi: 10.1117/12.459855
Proc. SPIE 4840, CELT site testing program, 0000 (30 January 2003); doi: 10.1117/12.459124
Proc. SPIE 4840, Dynamic modeling of turbulent shedding effect on the 30-m primary mirror of GSMT, 0000 (30 January 2003); doi: 10.1117/12.458038
Proc. SPIE 4840, Mach-Zehnder wavefront sensor for phasing of segmented telescopes, 0000 (30 January 2003); doi: 10.1117/12.458012
New Concepts and Ideas I
Proc. SPIE 4840, Optical issues for giant telescopes with extremely fast primary mirrors, 0000 (30 January 2003); doi: 10.1117/12.459934
Proc. SPIE 4840, Distributed pupil telescope designs, 0000 (30 January 2003); doi: 10.1117/12.459073
Proc. SPIE 4840, Giant segmented adaptive mirrors: progress report, 0000 (30 January 2003); doi: 10.1117/12.458176
New Concepts and Ideas II
Proc. SPIE 4840, Development of lightweight mirror elements for a very large astronomical adaptive optic primary mirror, 0000 (30 January 2003); doi: 10.1117/12.459929
Proc. SPIE 4840, Large-aperture mirror array (LAMA): conceptual design for a distributed-aperture 42-meter telescope, 0000 (30 January 2003); doi: 10.1117/12.459075
Proc. SPIE 4840, Large flexible membrane mirrors, 0000 (30 January 2003); doi: 10.1117/12.459059
Proc. SPIE 4840, New tools for a global survey of potential sites for the future giant telescopes, 0000 (30 January 2003); doi: 10.1117/12.459984
Proc. SPIE 4840, Critical science with the largest telescopes: science drivers for a 100-m ground-based optical-IR telescope, 0000 (30 January 2003); doi: 10.1117/12.458051
Poster Session
Proc. SPIE 4840, A 30-m Cassegrain telescope with spherical optics and a 3-deg. field, 0000 (30 January 2003); doi: 10.1117/12.459959
Proc. SPIE 4840, Analysis of efficiency of criterion of adaptation on the contrast of the infrared speckle image in large-sized telescopes, 0000 (30 January 2003); doi: 10.1117/12.459932
Proc. SPIE 4840, The Dittoscope, 0000 (30 January 2003); doi: 10.1117/12.459878
Proc. SPIE 4840, Edge effects with the Preston equation, 0000 (30 January 2003); doi: 10.1117/12.459869
Proc. SPIE 4840, Precision continuous high-strength azimuth track for large telescopes, 0000 (30 January 2003); doi: 10.1117/12.459070
Proc. SPIE 4840, Silicon anamorphic immersion gratings for IR high-resolution spectroscopy with future giant telescopes, 0000 (30 January 2003); doi: 10.1117/12.459064
General Interest
Proc. SPIE 4840, Estimating the costs of extremely large telescopes, 0000 (30 January 2003); doi: 10.1117/12.459868
Proc. SPIE 4840, New approach to enclosure design for large telescopes, 0000 (30 January 2003); doi: 10.1117/12.457988
Proc. SPIE 4840, Ultra-lightweight 4-m segmented composite mirrors for extremely large telescopes, 0000 (30 January 2003); doi: 10.1117/12.459865
Proc. SPIE 4840, SCOWL: a large format submillimeter camera on the Overwhelmingly Large Telescope, 0000 (30 January 2003); doi: 10.1117/12.458067
Proc. SPIE 4840, Mechanical design considerations unique to giant telescopes, 0000 (30 January 2003); doi: 10.1117/12.457995