東華大學圖書館 |

Language: English

Help

回圖書館首頁

手機版館藏查詢

Back

Switch To: Labeled | MARC Mode | ISBD

Development of coherent detector tec...

Tan, Boon Kok.

Linked to FindBook

Google Book

Amazon

博客來

Development of coherent detector technologies for sub-millimetre wave astronomy observations

Record Type:	Electronic resources : Monograph/item
Title/Author:	Development of coherent detector technologies for sub-millimetre wave astronomy observations/ by Boon-Kok Tan.
Author:	Tan, Boon Kok.
Published:	Cham :Springer International Publishing : : 2016.,
Description:	xxiv, 219 p. :ill., digital ;24 cm.
[NT 15003449]:	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.
Contained By:	Springer eBooks
Subject:	Submillimeter astronomy. -
Online resource:	http://dx.doi.org/10.1007/978-3-319-19363-2
ISBN:	9783319193632$q(electronic bk.)

Development of coherent detector technologies for sub-millimetre wave astronomy observations
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$q(electronic bk.)

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

2180502
Submillimeter astronomy.

LC Class. No.: QB479.4

Dewey Class. No.: 522.682

Development of coherent detector technologies for sub-millimetre wave astronomy observations
LDR:02792nmm a2200337 a 4500 001 2029461
003 DE-He213
005 20160801134155.0
006 m d
007 cr nn 008maaau
008 160908s2016 gw s 0 eng d
020 $a 9783319193632$q(electronic bk.)
020 $a 9783319193625$q(paper)
024 7 $a 10.1007/978-3-319-19363-2 $2 doi
035 $a 978-3-319-19363-2
040 $a GP $c GP
041 0 $a eng
050 4 $a QB479.4
072 7 $a PG $2 bicssc
072 7 $a SCI004000 $2 bisacsh
072 7 $a NAT033000 $2 bisacsh
082 0 4 $a 522.682 $2 23
090 $a QB479.4 $b .T161 2016
100 1 $a Tan, Boon Kok. $3 2180501
245 1 0 $a Development of coherent detector technologies for sub-millimetre wave astronomy observations $h [electronic resource] / $c by Boon-Kok Tan.
260 $a Cham : $b Springer International Publishing : $b Imprint: Springer, $c 2016.
300 $a xxiv, 219 p. : $b ill., digital ; $c 24 cm.
490 1 $a Springer theses, $x 2190-5053
505 0 $a 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.
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.
650 0 $a Submillimeter astronomy. $3 2180502
650 1 4 $a Physics. $3 516296
650 2 4 $a Astronomy, Observations and Techniques. $3 1066822
650 2 4 $a Optics, Optoelectronics, Plasmonics and Optical Devices. $3 1066388
710 2 $a SpringerLink (Online service) $3 836513
773 0 $t Springer eBooks
830 0 $a Springer theses. $3 1314442
856 4 0 $u http://dx.doi.org/10.1007/978-3-319-19363-2
950 $a Physics and Astronomy (Springer-11651)