论文信息 - Interferometry at mid-infrared wavelengths: the ISI system

Interferometry at mid-infrared wavelengths: the ISI system

The ISI (Infrared Spatial Interferometer) involves three movable telescopes of Pfund design, each in trailers, each with a radiation collecting mirror 65 inches in diameter. The telescopes can be moved, and then set down on concrete pads for stability. They are located on Mt. Wilson, where pads have been arranged to give baselines varying from 4 to approximately 75 meters and oriented in various directions. Initial work, between 1988 and 2002, was done with two telescopes; the third telescope was added in 2003.

Charles H. Townes | Edward H. Wishnow

[1] P. Tuthill,et al. Precision Measurements of the Diameters of α Orionis and ο Ceti at 11 Microns , 2000 .

[2] K. Tatebe,et al. Interferometry on stars at mid-infrared wavelengths , 2007, SPIE Optical Engineering + Applications.

[3] D W.C.,et al. MID-INFRARED INTERFEROMETRY ON SPECTRAL LINES . III . AMMONIA AND SILANE AROUND IRC ] 10216 AND VY CANIS , 2000 .

[4] William C. Danchi,et al. Multiple Dust Shells and Motions around IK Tauri as Seen by Infrared Interferometry , 1997 .

[5] W. J. Tango,et al. Very High Angular Resolution Imaging , 1994 .

[6] A. Michelson,et al. Measurement of the diameter of α Orionis with the interferometer , 1991 .

[7] William C. Danchi,et al. An IR spatial interferometer at 10 μm wavelength and measurement of stellar dust shells , 1994 .

[8] Rafael Millan-Gabet,et al. Michigan Infrared Combiner (MIRC): commissioning results at the CHARA Array , 2006, SPIE Astronomical Telescopes + Instrumentation.

[9] P. Strevens. Iii , 1985 .

[10] William C. Danchi,et al. Heterodyne Interferometry in the Infrared , 1994 .

[11] William C. Danchi,et al. Infrared Spatial Interferometer , 1998, Astronomical Telescopes and Instrumentation.