Published December 21, 2012
| Version v1
Journal article
The new RF sources for accelerators
Creators
- 1. Communications and Power Industries, LLC., 811 Hansen Way, Palo Alto, CA94304 (United States)
- 2. Calabazas Creek Research, Inc., 690 Port Drive, San Mateo, CA, 94404, (650) 312-9575 (United States)
Description
Several new RF sources are being developed for accelerator and collider applications. Assembly is nearing completion of a multiple beam inductive output tube at 352 MHz. An annular beam klystron is being developed to produce 10 MW pulses at 1.3 GHz. The annular beam approach provides significant cost reduction over similar multiple beam devices. Fabrication is underway on a 10 kW, periodic permanent magnet klystron at 2.815 GHz. Permanent magnets eliminate the solenoid and associated power supplies and cooling requirements to reduce operational cost. Investigations are beginning on a novel approach for driving accelerator cavities using pulse shaping to increase coupling efficiency and dramatically reduce RF power requirements.
Additional details
Identifiers
- DOI
- 10.1063/1.4773738;
Publishing Information
- Journal Title
- AIP Conference Proceedings
- Journal Volume
- 1507
- Journal Issue
- 1
- Journal Page Range
- p. 446-451
- ISSN
- 0094-243X
- CODEN
- APCPCS
Conference
- Title
- 15. advanced accelerator concepts workshop
- Dates
- 10-15 Jun 2012
- Place
- Austin, TX (United States)
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 44034956
- Subject category
- S43: PARTICLE ACCELERATORS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ACCELERATORS; CAVITY RESONATORS; GHZ RANGE; KLYSTRONS; MHZ RANGE; PARTICLE BEAMS; PERIODICITY; PERMANENT MAGNETS; POWER SUPPLIES; PULSES; RF SYSTEMS; SOLENOIDS
- Descriptors DEC
- BEAMS; ELECTRIC COILS; ELECTRICAL EQUIPMENT; ELECTRON TUBES; ELECTRONIC EQUIPMENT; EQUIPMENT; FREQUENCY RANGE; MAGNETS; MICROWAVE EQUIPMENT; MICROWAVE TUBES; RESONATORS; VARIATIONS
Optional Information
- Notes
- (c) 2012 American Institute of Physics