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Tsukanov, V.M.

Paper Title Page
THDO07

 The New VME-based System For Magnetic Measurements With Hall Sensors 

  • A.Batrakov, P.Vobly, S.Zverev, I.Ilyin, V.Kozak, E. Kuper, V.Mamkin V.Ovchar, G.Fatkin, V.M.Tsukanov, A.Volkov
    Budker Institute of Nuclear Physics, Novosibirsk, Russia

In BINP for creation of measuring systems with Hall sensors CAMAC - electronics were used many years. This system had good parameters and successfully used for measurements of magnets produced in BINP as for installations of VEPP-family as for foreign facilities: LHC (CERN), SLS (Switzerland), BESSY (Germany), SAGA (Japan). Hardware deterioration and MS DOS application of previous system demanded to design a new electronics and modern software. The paper describes the new VME-based system and MS Windows application developed for replacement of old system. The system hardware consists of VME crate controller, VME - RS-232 interface, VME - CAN interface and three specialized units: Hall-Sensor analogue Interface (VMEHSI), precision ADC (VMEADC16) and Hall carriage Thermo Stabilizer (HTS), fabricated in Budker INP. Resolution of measuring devices is less than 1uV and stability is better than 10-5. Software of the Hall-sensor measuring system consists of embedded part, which operates on VME-controller under the mcLinux operational system, and user's high-level software "WinHall", which is a MS Windows application with user-friendly graphical interface. The features of new system and practice results are reported.

55

MONP03

 3.5 Tesla 49-pole Superconducting Wiggler for DLS 

  • S.Khrushchev, V. Lev, N.Mezentsev, E. Miginsky, V. Repkov, V. Shkaruba, V. Syrovatin, V.M. Tsukanov
    Budker Institute of Nuclear Physics, Novosibirsk, Russia

3.5 Tesla 49-pole superconducting wiggler with 16 mm magnetic gap and 60 mm period for Diamond Light Source (England) has been fabricated in Budker INP. A first wiggler test was carried out in bath cryostat in BINP on July 2005. The first wiggler test in own cryostat was performed in BINP on January 2006. This test includes field integrals measurements with stretched wire method and field measurements with hall probe. All this measurements was repeated on April 2006 in DLS. Design of special magnetic measurement system with anti-chamber and main wiggler tests results are presented in this paper.

398

MONP06

 

 The Main Test Results Of The 3.5 Tesla 49-Pole Superconducting Wiggler for DLS 

  • E. Bekhtenev, S. Khrushchev, N. Mezentsev, E. Miginsky, V. Shkaruba, V.M. Tsukanov,
    BINP, Novosibirsk, Russia

3.5 Tesla 49-pole superconducting wiggler with 16 mm magnetic gap and 60 mm period for Diamond Light Source (England) has been fabricated in Budker INP. A first wiggler test was carried out in bath cryostat in BINP on July 2005. The first wiggler test in own cryostat was performed in BINP on January 2006. This test includes field integrals measurements with stretched wire method and field measurements with hall probe. All this measurements were repeated on April 2006 in DLS. Design of special magnetic measurement system with anti-chamber and main wiggler tests results are presented in this paper.

404

MODP23

 Temperature Stabilization of RF-cavities of VEPP-4M Electron-Positron Facility  

  • E.G.Miginskaya, I.I.Morozov, V.M.Tsukanov, A.A.Volkov
    Budker Institute of Nuclear Physics, Novosibirsk, Russia

Temperature variation of RF-cavities leads to a change of their geometrical sizes that provides undesirable cavity modes and to excitation of phase oscillations. It leads to decrease in luminosity and a beam life time. Flowing water heaters with stabilization of temperature have been established for elimination of this disadvantage. Temperature probes LM335 were used with a sensitivity of 10 μΒ per degree. The power part is made on the controllable switches CPV240. The analysis of temperature of input and output temperatures of water is carried out by microcontroller ADAM connected to a computer by means of interface RS-485. The temperature variation have been reduced from 5 to 0.2 degrees centigrade. That has led to decrease in probability of occurrence of parasitical phase oscillations more than in 100 times.