isi.ssl.berkeley.edu

The UC Berkeley Infrared Spatial Interferometer

The UC. Berkeley. Infrared Spatial Interferometer Array. Welcome to the U.C. Berkeley Infrared Spatial Interferometer Array. The ISI Array is a high resolution interferometer built by the Space Sciences Laboratory. At the University of California at Berkeley. California and is used for studying the properties of stars and immediate stellar environments in the mid-infrared. Portion of the spectrum. The ISI consists of three specially designed Pfund-type movable. Last update: 2009 June 10.

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The UC Berkeley Infrared Spatial Interferometer | isi.ssl.berkeley.edu Reviews

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The UC. Berkeley. Infrared Spatial Interferometer Array. Welcome to the U.C. Berkeley Infrared Spatial Interferometer Array. The ISI Array is a high resolution interferometer built by the Space Sciences Laboratory. At the University of California at Berkeley. California and is used for studying the properties of stars and immediate stellar environments in the mid-infrared. Portion of the spectrum. The ISI consists of three specially designed Pfund-type movable. Last update: 2009 June 10.

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The UC Berkeley Infrared Spatial Interferometer | isi.ssl.berkeley.edu Reviews

https://isi.ssl.berkeley.edu

The UC. Berkeley. Infrared Spatial Interferometer Array. Welcome to the U.C. Berkeley Infrared Spatial Interferometer Array. The ISI Array is a high resolution interferometer built by the Space Sciences Laboratory. At the University of California at Berkeley. California and is used for studying the properties of stars and immediate stellar environments in the mid-infrared. Portion of the spectrum. The ISI consists of three specially designed Pfund-type movable. Last update: 2009 June 10.

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isi.ssl.berkeley.edu

1

ISI Photo Gallery

http://isi.ssl.berkeley.edu/photo_gallery.htm

The UC. Berkeley. Infrared Spatial Interferometer Array. Early morning light on the ISI 10m baseline. Meteor over an ISI telescope. Sunrise on the ISI Flat Mirror Siderostat. Parabola Mirror Removal - I. Parabola Mirror Removal - II. Parabola Mirror Removal - III. Mirror Handling Facilities at the 108-inch Aluminizing Lab. Removing the old aluminnum coating. A final inspection before entering the aluminizing chamber. The 108-inch aluminizing tank and diffusion pump. ISI on 32m baseline.

2

ISI System Overview

http://isi.ssl.berkeley.edu/system_overview.htm

The UC. Berkeley. Infrared Spatial Interferometer Array. II The Prototype Instrument (c.1970). III Early 2-tel ISI (c.1988). V Infrared Heterodyne Detection. IX The Limitations of Two Telescopes. X The New 3-Telescope ISI Array (c.2003). A more technical and comprehensive description of the ISI System has been written by Hale et al., ApJ 537:998-1012, 2000. Has an angular resolution in visible light of about 0.05 arcsec. This, by comparison, is about the angular size of Alpha Orionis. Where there is no a...

3

ISI Financial Supporters

http://isi.ssl.berkeley.edu/financial_support.htm

The UC. Berkeley. Infrared Spatial Interferometer Array. The Army Research Office. The National Science Foundation. The Office of Naval Research.

4

Links

http://isi.ssl.berkeley.edu/links.htm

The UC. Berkeley. Infrared Spatial Interferometer Array. The single most comprehensive source of all interferometry news and related links is found here. Other ISI-related and interferometry links:. ISI Atmospheric Turbulence Experiment. ISI Observes Comet SL9 Impact with Jupiter. Infrared SETI with the ISI. Keck Aperture Masking Project. Interferometry Data Exchange Format. John D. Monnier. Peter G. Tuthill. Miscellaneous links of possible interest:. The Mount Wilson Observatory.

5

ISI Team

http://isi.ssl.berkeley.edu/team.htm

The UC. Berkeley. Infrared Spatial Interferometer Array. Charles H. Townes. Principal investigator; interferometry; heterodyne detection systems; everything physical. Co-principal investigator; astronomical instrumentation, infrared spectroscopy, interferometry. Electrical engineering; RF correlators and delay lines; everything analog. Assistant specialist; ISI operations. Systems engineer; wideband digital correlator. Network and real-time computer consultant. Nishanth Ranga Reddy P.

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iau-c54.wikispaces.com

IAU Commission 54: Optical Interferometry - Links

http://iau-c54.wikispaces.com/Links

Skip to main content. Get your brand new Wikispaces Classroom now. And do "back to school" in style. IAU Commission 54: Optical Interferometry. 2014 Interferometry Forum - Directions. LONG BASELINE STELLAR INTERFEROMETERS. Center for High Angular Resolution Astronomy Array ( Mnt Wilson. The CHARA Array hosts VEGA. Observatoire de la Cote d'Azur) and FLUOR. Fiber Linked Unit for Optical Recombination ( LESIA, Obs. de Paris. France) as well as MIRC (Michigan InfraRed Combiner). 10 microns) and LINC. Infrar...

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The UC Berkeley Infrared Spatial Interferometer

The UC. Berkeley. Infrared Spatial Interferometer Array. Welcome to the U.C. Berkeley Infrared Spatial Interferometer Array. The ISI Array is a high resolution interferometer built by the Space Sciences Laboratory. At the University of California at Berkeley. California and is used for studying the properties of stars and immediate stellar environments in the mid-infrared. Portion of the spectrum. The ISI consists of three specially designed Pfund-type movable. Last update: 2009 June 10.

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