Alternative optics design for the ALMA band 1 receiver (35-52 GHz)

Alvaro Gonzalez; Valeria Tapia; Ricardo Finger; Shin'Ichiro Asayama; Ted Huang

Alternative optics design for the ALMA band 1 receiver (35-52 GHz)

Alvaro Gonzalez
, Valeria Tapia
, Ricardo Finger
, Shin'Ichiro Asayama
, Ted Huang

Onderzoeksoutput: Hoofdstuk in Boek/Rapport/Congresprocedure › Conferentiebijdrage › Academic › peer review

Samenvatting

The Atacama Millimeter/Sub-millimeter Array (ALMA) is one of the most powerful telescopes built to date. All the receivers that cover the 10 frequency bands (35-950 GHz) in ALMA must comply with stringent requirements in order to perform astronomical observations, in particular, low noise temperature and high aperture efficiency. The ALMA band 1 receiver optics (35-52 GHz) are composed of a corrugated horn antenna and a dielectric lens. They have proved difficult to design because of the large bandwidth to cover and truncation effects in cryostat apertures. This paper presents a design which meets the stringent ALMA requirements.

Originele taal-2	Engels
Titel	2015 9th European Conference on Antennas and Propagation, EuCAP 2015
Plaats van productie	Piscataway
Uitgeverij	Institute of Electrical and Electronics Engineers
Aantal pagina's	4
ISBN van elektronische versie	978-8-8907-0185-6
Status	Gepubliceerd - 27 aug. 2015
Extern gepubliceerd	Ja
Evenement	9th European Conference on Antennas and Propagation (EuCAP 2015) - Lisbon, Portugal Duur: 13 mei 2015 → 17 mei 2015 Congresnummer: 9 http://www.eucap2015.org/

Congres

Congres	9th European Conference on Antennas and Propagation (EuCAP 2015)
Verkorte titel	EuCAP 2015
Land/Regio	Portugal
Stad	Lisbon
Periode	13/05/15 → 17/05/15
Ander	9th European Conference on Antennas and Propagation
Internet adres	http://www.eucap2015.org/

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@inproceedings{d3fea91c6a40444f80027caa092dd905,

title = "Alternative optics design for the ALMA band 1 receiver (35-52 GHz)",

abstract = "The Atacama Millimeter/Sub-millimeter Array (ALMA) is one of the most powerful telescopes built to date. All the receivers that cover the 10 frequency bands (35-950 GHz) in ALMA must comply with stringent requirements in order to perform astronomical observations, in particular, low noise temperature and high aperture efficiency. The ALMA band 1 receiver optics (35-52 GHz) are composed of a corrugated horn antenna and a dielectric lens. They have proved difficult to design because of the large bandwidth to cover and truncation effects in cryostat apertures. This paper presents a design which meets the stringent ALMA requirements.",

keywords = "lens, mm-wave antenna, Radio astronomy",

author = "Alvaro Gonzalez and Valeria Tapia and Ricardo Finger and Shin'Ichiro Asayama and Ted Huang",

year = "2015",

month = aug,

day = "27",

language = "English",

booktitle = "2015 9th European Conference on Antennas and Propagation, EuCAP 2015",

publisher = "Institute of Electrical and Electronics Engineers",

address = "United States",

note = "9th European Conference on Antennas and Propagation (EuCAP 2015), EuCAP 2015 ; Conference date: 13-05-2015 Through 17-05-2015",

url = "http://www.eucap2015.org/",

}

Gonzalez, A, Tapia, V, Finger, R, Asayama, SI & Huang, T 2015, Alternative optics design for the ALMA band 1 receiver (35-52 GHz). in 2015 9th European Conference on Antennas and Propagation, EuCAP 2015., 7228611, Institute of Electrical and Electronics Engineers, Piscataway, 9th European Conference on Antennas and Propagation (EuCAP 2015), Lisbon, Portugal, 13/05/15. <https://ieeexplore.ieee.org/document/7228611>

Alternative optics design for the ALMA band 1 receiver (35-52 GHz). / Gonzalez, Alvaro; Tapia, Valeria; Finger, Ricardo et al.
2015 9th European Conference on Antennas and Propagation, EuCAP 2015. Piscataway: Institute of Electrical and Electronics Engineers, 2015. 7228611.

Onderzoeksoutput: Hoofdstuk in Boek/Rapport/Congresprocedure › Conferentiebijdrage › Academic › peer review

TY - GEN

T1 - Alternative optics design for the ALMA band 1 receiver (35-52 GHz)

AU - Gonzalez, Alvaro

AU - Tapia, Valeria

AU - Finger, Ricardo

AU - Asayama, Shin'Ichiro

AU - Huang, Ted

N1 - Conference code: 9

PY - 2015/8/27

Y1 - 2015/8/27

N2 - The Atacama Millimeter/Sub-millimeter Array (ALMA) is one of the most powerful telescopes built to date. All the receivers that cover the 10 frequency bands (35-950 GHz) in ALMA must comply with stringent requirements in order to perform astronomical observations, in particular, low noise temperature and high aperture efficiency. The ALMA band 1 receiver optics (35-52 GHz) are composed of a corrugated horn antenna and a dielectric lens. They have proved difficult to design because of the large bandwidth to cover and truncation effects in cryostat apertures. This paper presents a design which meets the stringent ALMA requirements.

AB - The Atacama Millimeter/Sub-millimeter Array (ALMA) is one of the most powerful telescopes built to date. All the receivers that cover the 10 frequency bands (35-950 GHz) in ALMA must comply with stringent requirements in order to perform astronomical observations, in particular, low noise temperature and high aperture efficiency. The ALMA band 1 receiver optics (35-52 GHz) are composed of a corrugated horn antenna and a dielectric lens. They have proved difficult to design because of the large bandwidth to cover and truncation effects in cryostat apertures. This paper presents a design which meets the stringent ALMA requirements.

KW - lens

KW - mm-wave antenna

KW - Radio astronomy

UR - https://www.scopus.com/pages/publications/84949642522

M3 - Conference contribution

AN - SCOPUS:84949642522

BT - 2015 9th European Conference on Antennas and Propagation, EuCAP 2015

PB - Institute of Electrical and Electronics Engineers

CY - Piscataway

T2 - 9th European Conference on Antennas and Propagation (EuCAP 2015)

Y2 - 13 May 2015 through 17 May 2015

ER -

Alternative optics design for the ALMA band 1 receiver (35-52 GHz)

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