Presentation	1996/12/12 Array Configuration of Large Radio Interferometers for Astronomical Observations Koh-Ichiro Morita,
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Abstract(in Japanese)	(See Japanese page)
Abstract(in English)	Current configuration plan of the Large Millimeter and Submillimeter Array (LMSA) is based on five arrays ranging from 100 m to 10 km. The 10 km array has 0.01" which is better than that of Hubble Space Telescope. A most compact array will be used for high sensitivity survey observations and wide field observations. LMSA will have three intermediate configurations of which dimensions are -250 m, -70O m, and 2,000 m, so that we will have resolution jumping by factor of almost 3.0 for various astronomical requirements. Shape of each array configuration has not decided yet, but imaging simulations have suggested that centrally condensed Fourier coverate has better imaging performance for sparse configurations.
Keyword(in Japanese)	(See Japanese page)
Keyword(in English)	Interferometer / Radio Astronomy / Array configuration / Large Millimeter and Submillimeter Array
Paper #	A・P96-99
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Conference Information
Committee	AP
Conference Date	1996/12/12(1days)
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Place (in English)
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Paper Information
Registration To	Antennas and Propagation (A・P)
Language	JPN
Title (in Japanese)	(See Japanese page)
Sub Title (in Japanese)	(See Japanese page)
Title (in English)	Array Configuration of Large Radio Interferometers for Astronomical Observations
Sub Title (in English)
Keyword(1)	Interferometer
Keyword(2)	Radio Astronomy
Keyword(3)	Array configuration
Keyword(4)	Large Millimeter and Submillimeter Array
1st Author's Name	Koh-Ichiro Morita
1st Author's Affiliation	Nobeyama Radio Observatory, National Astronomical Observatory()
Date	1996/12/12
Paper #	A・P96-99
Volume (vol)	vol.96
Number (no)	400
Page	pp.pp.-
#Pages	7
Date of Issue