Nelson, 2008 - Google Patents
Thirty-Meter Telescope: progress and approachesNelson, 2008
- Document ID
- 16969074253296501430
- Author
- Nelson J
- Publication year
- Publication venue
- Extremely Large Telescopes: Which Wavelengths? Retirement Symposium for Arne Ardeberg
External Links
Snippet
I describe the design of the Thirty Meter Telescope, a project to build a ground-based thirty- meter telescope. The partners include the University of California, Caltech, the Association of Canadian Universities for Research in Astronomy (ACURA), and NSF. The Project is …
- 238000010276 construction 0 abstract description 7
Classifications
-
- G—PHYSICS
- G02—OPTICS
- G02B—OPTICAL ELEMENTS, SYSTEMS, OR APPARATUS
- G02B26/00—Optical devices or arrangements using movable or deformable optical elements for controlling the intensity, colour, phase, polarisation or direction of light, e.g. switching, gating, modulating
- G02B26/06—Optical devices or arrangements using movable or deformable optical elements for controlling the intensity, colour, phase, polarisation or direction of light, e.g. switching, gating, modulating for controlling the phase of light
-
- G—PHYSICS
- G02—OPTICS
- G02B—OPTICAL ELEMENTS, SYSTEMS, OR APPARATUS
- G02B26/00—Optical devices or arrangements using movable or deformable optical elements for controlling the intensity, colour, phase, polarisation or direction of light, e.g. switching, gating, modulating
- G02B26/08—Optical devices or arrangements using movable or deformable optical elements for controlling the intensity, colour, phase, polarisation or direction of light, e.g. switching, gating, modulating for controlling the direction of light
- G02B26/0816—Optical devices or arrangements using movable or deformable optical elements for controlling the intensity, colour, phase, polarisation or direction of light, e.g. switching, gating, modulating for controlling the direction of light by means of one or more reflecting elements
-
- G—PHYSICS
- G01—MEASURING; TESTING
- G01J—MEASUREMENT OF INTENSITY, VELOCITY, SPECTRAL CONTENT, POLARISATION, PHASE OR PULSE CHARACTERISTICS OF INFRA-RED, VISIBLE OR ULTRA-VIOLET LIGHT; COLORIMETRY; RADIATION PYROMETRY
- G01J3/00—Spectrometry; Spectrophotometry; Monochromators; Measuring colour
- G01J3/28—Investigating the spectrum
- G01J3/2823—Imaging spectrometer
-
- G—PHYSICS
- G01—MEASURING; TESTING
- G01J—MEASUREMENT OF INTENSITY, VELOCITY, SPECTRAL CONTENT, POLARISATION, PHASE OR PULSE CHARACTERISTICS OF INFRA-RED, VISIBLE OR ULTRA-VIOLET LIGHT; COLORIMETRY; RADIATION PYROMETRY
- G01J3/00—Spectrometry; Spectrophotometry; Monochromators; Measuring colour
- G01J3/12—Generating the spectrum; Monochromators
-
- G—PHYSICS
- G01—MEASURING; TESTING
- G01J—MEASUREMENT OF INTENSITY, VELOCITY, SPECTRAL CONTENT, POLARISATION, PHASE OR PULSE CHARACTERISTICS OF INFRA-RED, VISIBLE OR ULTRA-VIOLET LIGHT; COLORIMETRY; RADIATION PYROMETRY
- G01J3/00—Spectrometry; Spectrophotometry; Monochromators; Measuring colour
- G01J3/02—Details
- G01J3/0205—Optical elements not provided otherwise, e.g. optical manifolds, diffusers, windows
-
- G—PHYSICS
- G02—OPTICS
- G02B—OPTICAL ELEMENTS, SYSTEMS, OR APPARATUS
- G02B23/00—Telescopes, e.g. binoculars; Periscopes; Instruments for viewing the inside of hollow bodies; Viewfinders; Optical aiming or sighting devices
- G02B23/02—Telescopes, e.g. binoculars; Periscopes; Instruments for viewing the inside of hollow bodies; Viewfinders; Optical aiming or sighting devices involving prisms or mirrors
-
- G—PHYSICS
- G02—OPTICS
- G02B—OPTICAL ELEMENTS, SYSTEMS, OR APPARATUS
- G02B5/00—Optical elements other than lenses
-
- G—PHYSICS
- G02—OPTICS
- G02B—OPTICAL ELEMENTS, SYSTEMS, OR APPARATUS
- G02B17/00—Systems with reflecting surfaces, with or without refracting elements
- G02B17/02—Catoptric systems, e.g. image erecting and reversing system
- G02B17/06—Catoptric systems, e.g. image erecting and reversing system using mirrors only, i.e. having only one curved mirror
- G02B17/0605—Catoptric systems, e.g. image erecting and reversing system using mirrors only, i.e. having only one curved mirror using two curved mirrors
- G02B17/061—Catoptric systems, e.g. image erecting and reversing system using mirrors only, i.e. having only one curved mirror using two curved mirrors on-axis systems with at least one of the mirrors having a central aperture
-
- G—PHYSICS
- G02—OPTICS
- G02B—OPTICAL ELEMENTS, SYSTEMS, OR APPARATUS
- G02B27/00—Other optical systems; Other optical apparatus
- G02B27/42—Diffraction optics, i.e. systems including a diffractive element being designed for providing a diffractive effect
- G02B27/4205—Diffraction optics, i.e. systems including a diffractive element being designed for providing a diffractive effect having a diffractive optical element [DOE] contributing to image formation, e.g. whereby modulation transfer function MTF or optical aberrations are relevant
Similar Documents
| Publication | Publication Date | Title |
|---|---|---|
| Nelson et al. | The status of the Thirty Meter Telescope project | |
| Bond et al. | Adaptive optics with an infrared pyramid wavefront sensor at Keck | |
| Johns | The giant magellan telescope (GMT) | |
| Johns et al. | Giant magellan telescope: overview | |
| Cheng | The principles of astronomical telescope design | |
| Sheinis et al. | ESI, a new Keck Observatory echellette spectrograph and imager | |
| Padovani et al. | The extremely large telescope | |
| Nelson et al. | TMT status report | |
| Bouchez et al. | An overview and status of GMT active and adaptive optics | |
| Johns et al. | Status of the giant magellan telescope (GMT) project | |
| Thatte et al. | HARMONI: a single-field wide-band integral-field spectrograph for the European ELT | |
| Garcia-Mejia et al. | The Tierras Observatory: An ultra-precise photometer to characterize nearby terrestrial exoplanets | |
| Lloyd-Hart et al. | Design of the adaptive optics systems for GMT | |
| Strom et al. | Giant Segmented Mirror Telescope: a point design based on science drivers | |
| Nelson | Thirty-Meter Telescope: progress and approaches | |
| Shectman et al. | GMT overview | |
| Kim et al. | Optical technology for future telescopes | |
| Breckinridge et al. | Exoplanet telescope diffracted light minimized: the pinwheel-pupil solution | |
| Hill et al. | Present and future instrumentation for the Hobby-Eberly Telescope | |
| Lloyd-Hart et al. | Adaptive optics for the 6.5-m MMT | |
| Chun et al. | imaka: a path-finder ground-layer adaptive optics system for the University of Hawaii 2.2-meter telescope on Maunakea | |
| Rimmele et al. | Technical challenges of the advanced technology solar telescope | |
| Savage et al. | Current status of the Hobby-Eberly Telescope wide field upgrade and VIRUS | |
| Pirnay et al. | Mt ABU 2.5 m Telescope: design and fabrication | |
| Pirnay et al. | OAJ: 2.6 m wide field survey telescope |