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Radio-frequency power generation

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Radio-frequency power generation. / Carter, Richard G.
CERN Accelerator School: High Power Hadron Machines, CAS 2011 - Proceedings. CERN, 2013. p. 45-69 (CERN Accelerator School: High Power Hadron Machines, CAS 2011 - Proceedings).

Research output: Contribution in Book/Report/Proceedings - With ISBN/ISSNConference contribution/Paperpeer-review

Harvard

Carter, RG 2013, Radio-frequency power generation. in CERN Accelerator School: High Power Hadron Machines, CAS 2011 - Proceedings. CERN Accelerator School: High Power Hadron Machines, CAS 2011 - Proceedings, CERN, pp. 45-69, CERN Accelerator School: High Power Hadron Machines, CAS 2011, Bilbao, Spain, 24/05/11. https://doi.org/10.5170/CERN-2013-001.45

APA

Carter, R. G. (2013). Radio-frequency power generation. In CERN Accelerator School: High Power Hadron Machines, CAS 2011 - Proceedings (pp. 45-69). (CERN Accelerator School: High Power Hadron Machines, CAS 2011 - Proceedings). CERN. https://doi.org/10.5170/CERN-2013-001.45

Vancouver

Carter RG. Radio-frequency power generation. In CERN Accelerator School: High Power Hadron Machines, CAS 2011 - Proceedings. CERN. 2013. p. 45-69. (CERN Accelerator School: High Power Hadron Machines, CAS 2011 - Proceedings). doi: 10.5170/CERN-2013-001.45

Author

Carter, Richard G. / Radio-frequency power generation. CERN Accelerator School: High Power Hadron Machines, CAS 2011 - Proceedings. CERN, 2013. pp. 45-69 (CERN Accelerator School: High Power Hadron Machines, CAS 2011 - Proceedings).

Bibtex

@inproceedings{a91984005423467786acb116f924c935,
title = "Radio-frequency power generation",
abstract = "This paper reviews the main types of radio-frequency power amplifiers which are, or may be, used for high-power hadron accelerators. It covers tetrodes, inductive output tubes, klystrons and magnetrons with power outputs greater than 10 kW continuous wave or 100 kW pulsed at frequencies from 50 MHz to 30 GHz. Factors affecting the satisfactory operation of amplifiers include cooling, matching and protection circuits are discussed. The paper concludes with a summary of the state of the art for the different technologies.",
author = "Carter, {Richard G.}",
year = "2013",
month = sep,
day = "2",
doi = "10.5170/CERN-2013-001.45",
language = "English",
isbn = "9789290833840",
series = "CERN Accelerator School: High Power Hadron Machines, CAS 2011 - Proceedings",
publisher = "CERN",
pages = "45--69",
booktitle = "CERN Accelerator School",
note = "CERN Accelerator School: High Power Hadron Machines, CAS 2011 ; Conference date: 24-05-2011 Through 02-06-2011",

}

RIS

TY - GEN

T1 - Radio-frequency power generation

AU - Carter, Richard G.

PY - 2013/9/2

Y1 - 2013/9/2

N2 - This paper reviews the main types of radio-frequency power amplifiers which are, or may be, used for high-power hadron accelerators. It covers tetrodes, inductive output tubes, klystrons and magnetrons with power outputs greater than 10 kW continuous wave or 100 kW pulsed at frequencies from 50 MHz to 30 GHz. Factors affecting the satisfactory operation of amplifiers include cooling, matching and protection circuits are discussed. The paper concludes with a summary of the state of the art for the different technologies.

AB - This paper reviews the main types of radio-frequency power amplifiers which are, or may be, used for high-power hadron accelerators. It covers tetrodes, inductive output tubes, klystrons and magnetrons with power outputs greater than 10 kW continuous wave or 100 kW pulsed at frequencies from 50 MHz to 30 GHz. Factors affecting the satisfactory operation of amplifiers include cooling, matching and protection circuits are discussed. The paper concludes with a summary of the state of the art for the different technologies.

U2 - 10.5170/CERN-2013-001.45

DO - 10.5170/CERN-2013-001.45

M3 - Conference contribution/Paper

AN - SCOPUS:84883072864

SN - 9789290833840

T3 - CERN Accelerator School: High Power Hadron Machines, CAS 2011 - Proceedings

SP - 45

EP - 69

BT - CERN Accelerator School

PB - CERN

T2 - CERN Accelerator School: High Power Hadron Machines, CAS 2011

Y2 - 24 May 2011 through 2 June 2011

ER -