'Wfs' presentation slideshows

NGAO NGS WFS design review

NGAO NGS WFS design review. Caltech Optical Observatories 1 st April2010. Presentation outline. Requirements (including modes of operation and motion control) Introduction NGSWFS input feed (performance of the triplet and effect of atmospheric dispersion)

563 views • 45 slides

Fleet Administration Program & Processes

Fleet Administration Program & Processes. WHAT WFS DOES FOR YOU. Level 1 Services are for database administration of Airgas units. All units in the Airgas vehicle database receive level 1 services. Administration of the Airgas vehicle database Asset Input Asset Transfers Asset Retirements

463 views • 36 slides

Well-founded Semantics with Disjunction

411 views • 28 slides

Web Feature Server (WFS) Pilot Project

Web Feature Server (WFS) Pilot Project. Project Results and Demonstration Jonathan Doig - NSW Department of Land and Water Conservation Maurits van der Vlugt - Sinclair Knight Merz. Agenda. 3:30 Context, Purpose and Outcomes 3:45 Demonstration 4:10 Q&A - Discussion 4:30 End Session.

455 views • 25 slides

Pioneering GML Deployment for the NSDI

Pioneering GML Deployment for the NSDI. 2004 NSDI Cooperative Agreement Program Grant Project Category 5: Establishing Framework Data Services using the OGC Web Feature Service Specification. September 22, 2005 Jeff Harrison, President, The Carbon Project jharrison@thecarbonproject.com

368 views • 25 slides

Development of the first light AO system for Large Binocular Telescope

Development of the first light AO system for Large Binocular Telescope. S.Esposito, A.Tozzi, A.Puglisi, L.Fini, P.Stefanini, D.Gallieni, J.Storm,. Presented by Andrea Tozzi. SPIE Meeting, San Diego, August 04 th , 2003. Introduction.

382 views • 25 slides

Pioneering GML Deployment for the NSDI

Pioneering GML Deployment for the NSDI. 2004 NSDI Cooperative Agreement Program Grant Project Category 5: Establishing Framework Data Services using the OGC Web Feature Service Specification. September 22, 2005 Jeff Harrison, President, The Carbon Project jharrison@thecarbonproject.com

364 views • 25 slides

Adaptive Optics Requirements, Concepts, and Performance Predictions for Extremely Large Telescopes

Adaptive Optics Requirements, Concepts, and Performance Predictions for Extremely Large Telescopes. Brent Ellerbroek and Francois Rigaut Gemini Observatory SPIE Opto-Southwest / Astronomical Optics September 17, 2001. Presentation Outline. Requirements and AO operating modes

321 views • 20 slides

WFS 2.0 i Kortforsyningen

392 views • 20 slides

Adaptive Optics Requirements, Concepts, and Performance Predictions for Extremely Large Telescopes

Adaptive Optics Requirements, Concepts, and Performance Predictions for Extremely Large Telescopes. Brent Ellerbroek and Francois Rigaut Gemini Observatory SPIE Opto-Southwest / Astronomical Optics September 17, 2001. Presentation Outline. Requirements and AO operating modes

339 views • 20 slides

LGS wavefront sensor : Type and number of sub-apertures

379 views • 20 slides

The Angular Control System at LHO: Current Status

The Angular Control System at LHO: Current Status. Presented by Luca Matone LSC Conference at LHO Nov. 13 th , 2003. Paul Schwinberg, Stefan Ballmer, Matt Evans, Peter Fritschel, Nergis Mavalvala, Virginio Sannibale, Rick Savage, Daniel Sigg. Requirements.

279 views • 17 slides

Adaptive Optics Systems Engineering on GMT

Adaptive Optics Systems Engineering on GMT. Peter McGregor. Will GMT queue schedule instruments? What instrument configuration time is acceptable? Will GMT have general-purpose ports ? What field of view? Will the upper IP support non-AO instruments ? What field of view?

301 views • 16 slides

Design team reports: Wavefront sensors

Design team reports: Wavefront sensors. V. Velur , J. Bell, A. Moore, C. Neyman Design Meeting (Team meeting #10) Nov. 5 th , 2007. Agenda. WBS definition Inputs (as per WSPS) More input from science team, consensus from Systems team. Preliminary WFS design parameters and assumptions.

252 views • 12 slides

Infrared Wavefront Sensor (IR-WFS)

Infrared Wavefront Sensor (IR-WFS). Yutaka Hayano Internal Meeting on Future Instrument Projects at Subaru April 26, 2010. Why IR WFS. Highly obscured region. (No visible guide star.) Galactic center. Star forming region. Disks around massive YSOs

96 views • 9 slides