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Development of coherent detector technologies for sub-millimetre wave astronomy observations[electronic resource] /

紀錄類型:	書目-語言資料,印刷品 : Monograph/item
杜威分類號:	522.682
書名/作者:	Development of coherent detector technologies for sub-millimetre wave astronomy observations/ by Boon-Kok Tan.
作者:	Tan, Boon Kok.
出版者:	Cham : : Springer International Publishing :, 2016.
面頁冊數:	xxiv, 219 p. : : ill., digital ;; 24 cm.
Contained By:	Springer eBooks
標題:	Submillimeter astronomy.
標題:	Physics.
標題:	Astronomy, Observations and Techniques.
標題:	Optics, Optoelectronics, Plasmonics and Optical Devices.
ISBN:	9783319193632
ISBN:	9783319193625
內容註:	Introduction,- Multiple flare-angle smooth-walled horn -- SIS Mixer theory -- Design of unilateral finline SIS mixer -- Single-ended mixer tests -- Single-chip integrated balanced SIS mixer -- Design of 700 GHz single sideband SIS mixers -- The characteristics of an SIS junction near its superconducting gap -- Generation of local oscillator signal via photomixing -- CO (3→2) Observations of NGC 2976 and NGC 3351 -- Concluding remarks -- A Ancillary data of individual tested device -- B Ancillary data of individual tested balanced device -- C List of all beam patterns measured up to date -- D 230 GHz scalable design -- References.
摘要、提要註:	The thesis describes the development of receiver technologies for sub-millimetre astronomy instruments, focusing on high performance coherent cryogenic detectors operating close to the superconductor gap frequency. The mixer chip which comprises the SIS devices, fed by a unilateral finline and matching planar circuits was fabricated on 15 micron silicon substrate using the recently developed Silicon-On-Insulator (SOI) technology. This offered broadband IF and RF performance, with fully integrated on-chip planar circuits resulting in an easily reproducible mixer chip and a simple mixer block. An important consequence of this design is that it can be extended to the supra-THz region and making the fabrication of multi-pixel heterodyne arrays feasible. The extension of the operation of major telescopes such as ALMA, APEX and the GLT from single pixel to large format arrays is the subject of extensive research at present time since it will allow fast mapping combined with high resolution of the submillimetre sky. The technology described in this thesis makes a major contribution to this effort.
電子資源:	http://dx.doi.org/10.1007/978-3-319-19363-2

Development of coherent detector technologies for sub-millimetre wave astronomy observations[electronic resource] /
Tan, Boon Kok.

Development of coherent detector technologies for sub-millimetre wave astronomy observations[electronic resource] /by Boon-Kok Tan. - Cham :Springer International Publishing :2016. - xxiv, 219 p. :ill., digital ;24 cm. - Springer theses,2190-5053. - Springer theses..

Introduction,- Multiple flare-angle smooth-walled horn -- SIS Mixer theory -- Design of unilateral finline SIS mixer -- Single-ended mixer tests -- Single-chip integrated balanced SIS mixer -- Design of 700 GHz single sideband SIS mixers -- The characteristics of an SIS junction near its superconducting gap -- Generation of local oscillator signal via photomixing -- CO (3→2) Observations of NGC 2976 and NGC 3351 -- Concluding remarks -- A Ancillary data of individual tested device -- B Ancillary data of individual tested balanced device -- C List of all beam patterns measured up to date -- D 230 GHz scalable design -- References.

The thesis describes the development of receiver technologies for sub-millimetre astronomy instruments, focusing on high performance coherent cryogenic detectors operating close to the superconductor gap frequency. The mixer chip which comprises the SIS devices, fed by a unilateral finline and matching planar circuits was fabricated on 15 micron silicon substrate using the recently developed Silicon-On-Insulator (SOI) technology. This offered broadband IF and RF performance, with fully integrated on-chip planar circuits resulting in an easily reproducible mixer chip and a simple mixer block. An important consequence of this design is that it can be extended to the supra-THz region and making the fabrication of multi-pixel heterodyne arrays feasible. The extension of the operation of major telescopes such as ALMA, APEX and the GLT from single pixel to large format arrays is the subject of extensive research at present time since it will allow fast mapping combined with high resolution of the submillimetre sky. The technology described in this thesis makes a major contribution to this effort.

ISBN: 9783319193632

Standard No.: 10.1007/978-3-319-19363-2doiSubjects--Topical Terms:

653497
Submillimeter astronomy.

LC Class. No.: QB479.4

Dewey Class. No.: 522.682

Development of coherent detector technologies for sub-millimetre wave astronomy observations[electronic resource] /
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520 $a The thesis describes the development of receiver technologies for sub-millimetre astronomy instruments, focusing on high performance coherent cryogenic detectors operating close to the superconductor gap frequency. The mixer chip which comprises the SIS devices, fed by a unilateral finline and matching planar circuits was fabricated on 15 micron silicon substrate using the recently developed Silicon-On-Insulator (SOI) technology. This offered broadband IF and RF performance, with fully integrated on-chip planar circuits resulting in an easily reproducible mixer chip and a simple mixer block. An important consequence of this design is that it can be extended to the supra-THz region and making the fabrication of multi-pixel heterodyne arrays feasible. The extension of the operation of major telescopes such as ALMA, APEX and the GLT from single pixel to large format arrays is the subject of extensive research at present time since it will allow fast mapping combined with high resolution of the submillimetre sky. The technology described in this thesis makes a major contribution to this effort.
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