Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

Tuner of a Second Harmonic Cavity of the Fermilab Booster

Conference ·
OSTI ID:1366525

Introducing a second harmonic cavity in the accelerating system of the Fermilab Booster promises significant reduc-tion of the particle beam loss during the injection, transi-tion, and extraction stages. To follow the changing energy of the beam during acceleration cycles, the cavity is equipped with a tuner that employs perpendicularly biased AL800 garnet material as the frequency tuning media. The required tuning range of the cavity is from 75.73 MHz at injection to 105.64 MHz at extraction. This large range ne-cessitates the use of a relatively low bias magnetic field at injection, which could lead to high RF loss power density in the garnet, or a strong bias magnetic field at extraction, which could result in high power consumption in the tuner’s bias magnet. The required 15 Hz repetition rate of the device and high sensitivity of the local RF power loss to the level of the magnetic field added to the challenges of the bias system design. In this report, the main features of a proposed prototype of the second harmonic cavity tuner are presented.

Research Organization:
Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States)
Sponsoring Organization:
USDOE Office of Science (SC), High Energy Physics (HEP) (SC-25)
Contributing Organization:
PIP
DOE Contract Number:
AC02-07CH11359
OSTI ID:
1366525
Report Number(s):
FERMILAB-CONF-17-164-TD; IPAC-2017-THPIK113; 1607164
Country of Publication:
United States
Language:
English

Similar Records

Static Magnetic Properties of AL800 Garnet Material
Conference · Wed May 17 00:00:00 EDT 2017 · OSTI ID:1366524

Perpendicularly Biased YIG Tuners for the Fermilab Recycler 52.809 MHz Cavities
Conference · Fri Sep 13 00:00:00 EDT 2013 · OSTI ID:1128769

Measurements of the Properties of Garnet Material for Tuning a 2nd Harmonic Cavity for the Fermilab Booster
Conference · Thu Dec 31 23:00:00 EST 2015 · OSTI ID:1358093

Related Subjects