Zobrazeno 1 - 9
of 9
pro vyhledávání: '"Andy Kissil"'
Autor:
Doug Lisman, Andy Kissil, Marie Levine-West, Tim Ho, E. Y. Kwack, Phil Dumont, Terry Cafferty, Virginia G. Ford, Peter Feher
Publikováno v:
Proceedings of the International Astronomical Union. 1:335-344
Creating an optical space telescope observatory capable of detecting and characterizing light from extra-solar terrestrial planets poses technical challenges related to extreme wavefront stability. The Terrestrial Planet Finder Coronagraph design tea
Publikováno v:
AIAA Journal. 34:821-829
Mode shape expansion techniques fall under four broad categories. Spatial interpolation methods use geometric information to infer mode shapes at unmeasured locations. Direct methods use the dynamic equations of motion to obtain closed-form solutions
Autor:
Jeff Zolkower, Bruno Clavel, Eric Chauvin, Paul Rasmussen, David P. Woody, Andy Kissil, German Cortes, John Z. Lou, David C. Redding, S. Padin
CCAT will be a 25 m diameter telescope operating in the 2 to 0.2 mm wavelength range. It will be located at an altitude of 5600 m on Cerro Chajnantor in Northern Chile. The telescope will be equipped with wide-field, multi-color cameras for surveys a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::588baac7d3e2350df4f08e94cda99105
https://resolver.caltech.edu/CaltechAUTHORS:20130124-095627846
https://resolver.caltech.edu/CaltechAUTHORS:20130124-095627846
Publikováno v:
Integrated Modeling of Complex Optomechanical Systems.
The 25-m aperture CCAT submillimeter-wave telescope will have a primary mirror that is divided into 162 individual segments, each of which is provided with 3 positioning actuators. CCAT will be equipped with innovative Imaging Displacement Sensors (I
Publikováno v:
2011 XXXth URSI General Assembly and Scientific Symposium.
CCAT will be a 25 m diameter Ritchey-Chretien telescope operating in the 0.2–1.5 mm wavelength range. It will be located at an altitude of 5600 m on Cerro Chajnantor in northern Chile, near the ALMA site. CCAT will have an f/0.4 primary, with an ac
The 25 meter aperture Cornell Caltech Atacama Telescope (CCAT) will provide an enormous increase in sensitivity in the submillimeter bands compared to existing observatories, provided it can establish and maintain excellent image quality. To accompli
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0f2635c03ce1240cdc74dfee47d84128
https://resolver.caltech.edu/CaltechAUTHORS:20161108-133204295
https://resolver.caltech.edu/CaltechAUTHORS:20161108-133204295
The 25-m aperture Cornell Caltech Atacama Telescope (CCAT) will have a primary mirror that is divided into 162 individual segments, each of which is equipped with 3 positioning actuators. This paper presents a mathematical description of the telescop
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a2252938eb69cec47311eec13ea2108c
https://resolver.caltech.edu/CaltechAUTHORS:20161031-141458642
https://resolver.caltech.edu/CaltechAUTHORS:20161031-141458642
Publikováno v:
Control of Vibration and Noise: New Millennium.
The Space Interferometer Mission (SIM) scheduled for launch in 2008, is one of the premiere missions in the Origins Program, NASA’s endeavor to understand the origins of the galaxies, of planetary systems around distant stars, and perhaps the origi
Conference
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