skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Development of X-band klystron technology at SLAC

Conference ·
OSTI ID:525018

The SLAC design for a 1-TeV collider (NLC) requires klystrons with a performance which is well beyond the state-of-the-art for microwave tubes in the United States or abroad. The electrical specifications for the NLC klystrons are not fully established, but they are approximately as follows: Frequency, 11.4 GHz; Peak Power, 75 MW; Pulse Length, 1.5 {mu}s; Repetition Rate, 180 Hz; Gain, 50 dB; Efficiency, (including beam focusing) 50%. SLAC is in the seventh year of a program to develop these klystrons. The choice of X-band as the operating frequency, along with the sheer size of the NLC, have resulted in some new, most demanding standards for the klystrons which may power this future machine. These are related to the overall efficiency required, to the high rf gradients that must be supported at the output circuit without vacuum breakdown, and to the manufacturing cost of the 5,000-10,000 klystrons needed for the collider.

Research Organization:
SLAC National Accelerator Lab., Menlo Park, CA (United States)
Sponsoring Organization:
USDOE Office of Energy Research, Washington, DC (United States)
DOE Contract Number:
AC03-76SF00515
OSTI ID:
525018
Report Number(s):
SLAC-PUB-7548; CONF-970503-278; ON: DE97007341; TRN: 97:018514
Resource Relation:
Conference: 17. IEEE particle accelerator conference, Vancouver (Canada), 12-16 May 1997; Other Information: PBD: May 1997
Country of Publication:
United States
Language:
English

Similar Records

The X-band klystron program at SLAC
Conference · Mon Apr 01 00:00:00 EST 1996 · OSTI ID:525018

Periodic permanent magnet development for linear collider X-band klystrons
Journal Article · Fri May 07 00:00:00 EDT 1999 · AIP Conference Proceedings · OSTI ID:525018

Periodic permanent magnet development for linear collider X-band klystrons
Journal Article · Sat May 01 00:00:00 EDT 1999 · AIP Conference Proceedings · OSTI ID:525018