| Item type |
紀要論文 / Departmental Bulletin Paper(1) |
| 公開日 |
2015-03-26 |
| タイトル |
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|
タイトル |
The SPIRIT and SPECS Far-Infrared / Submillimeter Interferometry Missions |
|
言語 |
en |
| 言語 |
|
|
言語 |
eng |
| 資源タイプ |
|
|
資源タイプ識別子 |
http://purl.org/coar/resource_type/c_6501 |
|
資源タイプ |
departmental bulletin paper |
| 著者 |
MATHER, John C.
LEISAWITZ, David
The, Far-IR Interferometry Mission Study Working Group
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| 著者所属（英） |
|
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|
en |
|
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NASA Goddard Space Flight Center |
| 著者所属（英） |
|
|
|
en |
|
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NASA Goddard Space Flight Center |
| 著者所属（英） |
|
|
|
en |
|
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The Far-IR Interferometry Mission Study Working Group |
| 出版者 |
|
|
出版者 |
宇宙科学研究所 |
| 出版者（英） |
|
|
出版者 |
Institute of Space and Astronautical Science |
| 書誌情報 |
en : The Institute of Space and Astronautical Science report. S.P. : Mid- and Far-Infrared Astronomy and Future Space Mission
巻 14,
p. 219-224,
発行日 2000-12
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| 抄録（英） |
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内容記述タイプ |
Other |
|
内容記述 |
Space-based far IR/submillimeter (FIR/SMM) interferometry is needed to answerfundamental cosmological questions concerning the development of structure in the Universe andcould also be used to probe nearby objects such as protostars, young planetary systems, anddebris disks in unprecedented detail. We describe concepts for the Space Infrared InterferometricTelescope (SPIRIT) and the Submillimeter Probe of the Evolution of Cosmic Structure (SPECS).Both are imaging and spectral Michelson interferometers operating in the wavelength range ～40-500 μm. The individual light-collecting mirrors are comparable in size and temperature to theHII/L2 primary mirror. SPIRIT, which could be launched in a decade, is built on a deployableboom and has a maximum baseline of ～30-50 m, providing arcsecond resolution in the far-IR.SPECS uses formation flying to attain baseline lengths up to ～1 km, and thus angular resolutioncomparable to that of the Hubble Space Telescope (HST), the Next Generation Space Telescope(NGST), and the Atacama Large Millimeter Array (ALMA). SPIRIT and SPECS would provideaccess to many important cooling and diagnostic spectral lines and to the bulk of the thermalemission from dust, and make observations complementary to those obtained with ALMA andNGST. |
| ISSN |
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収録物識別子タイプ |
ISSN |
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収録物識別子 |
0288-433X |
| 書誌レコードID |
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収録物識別子タイプ |
NCID |
|
収録物識別子 |
AA10455137 |
| 資料番号 |
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内容記述タイプ |
Other |
|
内容記述 |
資料番号: SA4592253000 |
SA4592253.pdf (219.6 kB)
