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Balloon-borne Infrared Telescope (BIRT) for far-infrared spectroscopyThe Japanese-made Balloon-borne Infrared Telescope (BIRT) designed for FIR astronomy is described. The BIRT system includes a 50-cm-diam telescope; an attitude-control system consisting of an attitude stabilization and a pointing and tracking subsystems; the ground support system consisting of four personal-computer systems; and electronics consisting of three small computer systems, servo circuits, power amplifiers, and other small circuits. Between 1985 and 1988, the BIRT has flown eight times, demonstrating that it is able to provide a suitable telescope observations on a stable platform with a long integration time. Structural diagrams of the BIRT overall system, the optical system, and the wobbling mechanism are presented along with a block diagram of the on-board electronics.
Document ID
19910044990
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Shibai, Hiroshi
(Tokyo Univ. Sagamihara, Japan)
Okuda, Haruyuki
(Tokyo Univ. Sagamihara, Japan)
Nakagawa, Takao
(Tokyo Univ. Sagamihara, Japan)
Yajima, Nobuyuki
(Institute of Space and Astronautical Science Sagamihara, Japan)
Maihara, Toshinori
(Kyoto University Japan)
Date Acquired
August 14, 2013
Publication Date
January 1, 1990
Subject Category
Instrumentation And Photography
Meeting Information
Meeting: Instrumentation in Astronomy VII
Location: Tucson, AZ
Country: United States
Start Date: February 13, 1990
End Date: February 17, 1990
Sponsors: SPIE
Accession Number
91A29613
Funding Number(s)
CONTRACT_GRANT: NGR-03-002-269
CONTRACT_GRANT: NSF INT-86-13481
Distribution Limits
Public
Copyright
Other

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