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Title: The conversion of CESR to operate as the Test Accelerator, CesrTA. Part 3: Electron cloud diagnostics

Abstract

Cornell's electron/positron storage ring (CESR) was modified over a series of accelerator shutdowns beginning in May 2008, which substantially improves its capability for research and development for particle accelerators. CESR's energy span from 1.8 to 5.6 GeV with both electrons and positrons makes it ideal for the study of a wide spectrum of accelerator physics issues and instrumentation related to present light sources and future lepton damping rings. Additionally a number of these are also relevant for the beam physics of proton accelerators. This paper is the third in a series of four describing the conversion of CESR to the test accelerator, CESRTA. The first two papers discuss the overall plan for the conversion of the storage ring to an instrument capable of studying advanced accelerator physics issues [1] and the details of the vacuum system upgrades [2]. This paper focuses on the necessary development of new instrumentation, situated in four dedicated experimental regions, capable of studying such phenomena as electron clouds (ECs) and methods to mitigate EC effects. The fourth paper in this series describes the vacuum system modifications of the superconducting wigglers to accommodate the diagnostic instrumentation for the study of EC behavior within wigglers. Lastly, while themore » initial studies of CESRTA focused on questions related to the International Linear Collider damping ring design, CESRTA is a very versatile storage ring, capable of studying a wide range of accelerator physics and instrumentation questions.« less

Authors:
 [1];  [1];  [1];  [1];  [1];  [1];  [1];  [1];  [2];  [3]
+ Show Author Affiliations
  1. Cornell Univ., Ithaca, NY (United States)
  2. Argonne National Lab. (ANL), Lemont, IL (United States)
  3. Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
Publication Date:
Research Org.:
Argonne National Lab. (ANL), Argonne, IL (United States); Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
Sponsoring Org.:
USDOE Office of Science (SC), High Energy Physics (HEP)
OSTI Identifier:
1327423
Report Number(s):
arXiv:1512.00748; FERMILAB-PUB-16-404-APC
Journal ID: ISSN 1748-0221; 1407879
Grant/Contract Number:  
AC02-07CH11359
Resource Type:
Journal Article: Accepted Manuscript
Journal Name:
Journal of Instrumentation
Additional Journal Information:
Journal Volume: 11; Journal Issue: 04; Journal ID: ISSN 1748-0221
Publisher:
Institute of Physics (IOP)
Country of Publication:
United States
Language:
English
Subject:
43 PARTICLE ACCELERATORS; accelerator subsystems and technologies; instrumentation for particle accelerators and storage rings - high energy (linear accelerators, synchrotrons); detector design and construction technologies and materials; data acquisition circuits

Citation Formats

Billing, M. G., Conway, J. V., Crittenden, J. A., Greenwald, S., Li, Y., Meller, R. E., Strohman, C. R., Sikora, J. P., Calvey, J. R., and Palmer, M. A. The conversion of CESR to operate as the Test Accelerator, CesrTA. Part 3: Electron cloud diagnostics. United States: N. p., 2016. Web. doi:10.1088/1748-0221/11/04/P04025.
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Billing, M. G., Conway, J. V., Crittenden, J. A., Greenwald, S., Li, Y., Meller, R. E., Strohman, C. R., Sikora, J. P., Calvey, J. R., & Palmer, M. A. The conversion of CESR to operate as the Test Accelerator, CesrTA. Part 3: Electron cloud diagnostics. United States. https://doi.org/10.1088/1748-0221/11/04/P04025
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Billing, M. G., Conway, J. V., Crittenden, J. A., Greenwald, S., Li, Y., Meller, R. E., Strohman, C. R., Sikora, J. P., Calvey, J. R., and Palmer, M. A. 2016. "The conversion of CESR to operate as the Test Accelerator, CesrTA. Part 3: Electron cloud diagnostics". United States. https://doi.org/10.1088/1748-0221/11/04/P04025. https://www.osti.gov/servlets/purl/1327423.
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@article{osti_1327423,
title = {The conversion of CESR to operate as the Test Accelerator, CesrTA. Part 3: Electron cloud diagnostics},
author = {Billing, M. G. and Conway, J. V. and Crittenden, J. A. and Greenwald, S. and Li, Y. and Meller, R. E. and Strohman, C. R. and Sikora, J. P. and Calvey, J. R. and Palmer, M. A.},
abstractNote = {Cornell's electron/positron storage ring (CESR) was modified over a series of accelerator shutdowns beginning in May 2008, which substantially improves its capability for research and development for particle accelerators. CESR's energy span from 1.8 to 5.6 GeV with both electrons and positrons makes it ideal for the study of a wide spectrum of accelerator physics issues and instrumentation related to present light sources and future lepton damping rings. Additionally a number of these are also relevant for the beam physics of proton accelerators. This paper is the third in a series of four describing the conversion of CESR to the test accelerator, CESRTA. The first two papers discuss the overall plan for the conversion of the storage ring to an instrument capable of studying advanced accelerator physics issues [1] and the details of the vacuum system upgrades [2]. This paper focuses on the necessary development of new instrumentation, situated in four dedicated experimental regions, capable of studying such phenomena as electron clouds (ECs) and methods to mitigate EC effects. The fourth paper in this series describes the vacuum system modifications of the superconducting wigglers to accommodate the diagnostic instrumentation for the study of EC behavior within wigglers. Lastly, while the initial studies of CESRTA focused on questions related to the International Linear Collider damping ring design, CESRTA is a very versatile storage ring, capable of studying a wide range of accelerator physics and instrumentation questions.},
doi = {10.1088/1748-0221/11/04/P04025},
url = {https://www.osti.gov/biblio/1327423}, journal = {Journal of Instrumentation},
issn = {1748-0221},
number = 04,
volume = 11,
place = {United States},
year = {Thu Apr 28 00:00:00 EDT 2016},
month = {Thu Apr 28 00:00:00 EDT 2016}
}
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Journal Article:
Free Publicly Available Full Text
Publisher's Version of Record
https://doi.org/10.1088/1748-0221/11/04/P04025
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