Booster Neutrino Beamline Facility Operations Update Present & - - PowerPoint PPT Presentation

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Booster Neutrino Beamline Facility Operations Update Present & - - PowerPoint PPT Presentation

Booster Neutrino Beamline Facility Operations Update Present & Future Thomas R. Kobilarcik September 23, 2014 Neutrino Beams and Instrumentation, 2014 SEPTEMBER SUNDAY MONDAY TUESDAY WEDNESDAY THURSDAY FRIDAY SATURDAY 1 2 3 4 5


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Booster Neutrino Beamline Facility Operations Update Present & Future

Thomas R. Kobilarcik September 23, 2014 Neutrino Beams and Instrumentation, 2014

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  • Sept. 23, 2014

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SEPTEMBER

SUNDAY MONDAY TUESDAY WEDNESDAY THURSDAY FRIDAY SATURDAY

1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30

PRESENT

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MiniBooNE SciBooNE MicroBooNE Booster Neutrino Beamline Booster

Booster Neutrino Beamline and Detectors

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Primary Beamline

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The horns have pulsed half-a-billion times. Since turning

  • n, BNB has

transported 2.1E21 protons. BNB is assessed for 5×1012 protons per pulse at 5 Hz average.

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OLD Old instrumentation was able to keep beam

  • n target, measure

intensity, and measure beam width when needed. NEW New instrumentation employs low-mass multiwires, allowing continual monitoring of beam shape. Additionally, we are able to reference multiwires to external coordinate system, allowing us to locate beam position and trajectory in site coordinate system.

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Second generation low-mass multiwires. Welded joints, easy access to wire plane, more robust mechanical design. Separation between planes remains at 110 cm and planes retain 0.5 mm pitch. New instrumentation package will be installed when horn is changed.

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2 GHz sample rate over entire spill. Data is recorded every pulse, and is available through the Intensity Frontier Beam Database.

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BEAM

Service Building For Target and Horn Wells 25 m Absorber 50 m Absorber Berm Cooling System Wells

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Secondary Beamline and Associated Systems

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Target and Horn Assembley

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Designed by Larry Bartoszek Built by AD Mechanical Support Target Group Present engineer is Vladimir Sidorov Target and horn are built and installed as a single unit, although it is possible to change only the target.

  • Sept. 23, 2014

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First Horn April 28, 2002 to July 28, 2004 97 million pulses Both horn and target were replaced Suspected cause of failure was stagnant water in return line bellows.

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Unstack 6x15 shielding blocks. Blocks needed to be wrapped. Remove final focus triplet. Lower coffin. Remove horn. Reverse procedure. Shielding Target and Horn are buried in shielding. Approximately 12 weeks to change horn, most of which is removing shielding infrastructure. Target can be changed independently of horn. Horn

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Drainage tube removes stagnant water

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Second Horn Trivia

December 2004 to present. 1/3 of a billion pulses. Two of the six water lines have been valved out due to leakage, but still have adequate cooling. Provides new data regarding fatigue of aluminum. Water is continually circulated, even during shutdowns and

  • ff-target running, to avoid stagnation.
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Deployable absorber located 25 m from target. Absorber consists of nine one foot thick steel plates, one three foot thick concrete block, and one foot thick instrumented panel. Each module is ten feet wide and ten feet tall. Originally suspended with high-strength steel chains

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“problems” is an understatement. A number of chains failed due to hydrogen embrittlement. Several absorber modules fell into decay pipe. All chains were removed and replaced with steel rods.

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One absorber module is instrumented with loss monitors. Unfortunately, this is one of the modules that fell, and it is not known if the loss monitors still work. Each module consist of six two inch thick steel plates. The plates are welded together. The module is instrumented by cutting a cross is two of the plates (the second and third plates from the front). A slot to run the cables is also cut in the plates.

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The 50 m absorber has the same instrumentation as the 25 m absorber 8’ 8” of steel “blue blocks”, three feet of concrete (10’ by 10’), one instrumentation panel, and 26”

  • f steel (more “blue blocks”).
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The array of loss monitors is read back using the same electronics as we use for the profile monitors. Over time the signals have degraded. Because the system is buried, there is no access to it. Profile data is recorded in IF Beams database.

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Berm Cooling System

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Closed loop air system. Air is circulated through large HDPE pipes in

  • rder to remove heat

from berm.

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Only able to access cooling pipes through supply and return. Unable to inspect system once buried.

service building 25 m absorber 50 m absorber cooling pipes LMC

System was first used in 2013 for off-target running. Temperature probes were inserted through LMC pipe near absorber.

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Three drainage systems.

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Decay pipe buried in 12 to 15 feet of aggregate. Aggregate is surrounded by two impermeable liners. Each drain connects to two monitoring wells,

  • ne upstream and one

downstream. Expect water in exterior drain tile, but inner and interstitial drains should remain dry. Early on we found they did not, implying there is a leak in the liner

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service building liner upstream wells downstream wells

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Replacing the pump requires pulling the pump and pipe with a crane or lift bucket.

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Planned Facility Modifications

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Run beam off target. Hang two SWICs (Segmented Wire Ionization Chamber) upstream and downstream of 25 m absorber. This will allow one to tie the primary beam trajectory to the site coordinate system. This is a one-time measurement. Planned for this year, after the shutdown.

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Install impermeable barrier to keep water away from liner. Over the past year a temporary tarp was placed over the berm and adjoining area. This worked well in keeping water out of the tear. New barrier is permanent. About one foot of dirt will be remove, the barrier will be installed, and the dirt will be replaced. Drain tile will be installed around the toe

  • f the berm.

Work starts this week

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Possibilities …

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MiniBooNE SciBooNE MicroBooNE Booster Neutrino Beamline

Room for More Detectors

New Near Detector ? New Far Detector ?

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Modify first and last modules to contain retractable wire chambers. Due to how the absorber system is build,

  • ne would need to lower all the absorbers,

pull out the first and last modules, replace them with modified modules, then lift all back in place. Alignment would be challenging. drive mechanism drive rods wire chamber notched and slotted steel absorber

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Dig up and rebuild the 50 m absorber. Replace blue blocks with steel plates in order to eliminate cracks. Install a hadron monitor, similar to that in the NuMI beamline. Build a structure to allow access. This would be challenging. The liner would have to be opened and then resealed. The aggregate surrounding the absorber is

  • radioactive. The blue blocks are radioactive. However, this option

would allow one to know accurately the direction of the primary beam.

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NBI2014 -- T. Kobilarcik 36

Change target material. Change shape of inner conductor. Re-optimize horn. The present target and horn system is optimized for MiniBooNE. The target size and material can be changed to suit the need of future experiment. The shape of the inner conductor can also be changed.

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Add a second horn. But… Where do you put it?

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Steel shielding (red hatch) Final focusing triplet (light blue) Sump pit (blue circle) Concrete shielding blocks, which form part of the floor of the enclosure (green hatch) Most of this area is filled support infrastructure

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Use smaller magnets for triplet, which allows one to push beamline upstream? Fill free space in target hall with steel shielding? Move infrastructure into tunnel? How does one route the striplines for the second horn? Does one need to re-route striplines for the first horn? Where does one put the power supply for the second horn?

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Build a new beamline.

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Ending Comments

The Booster Neutrino Beamline has run successfully for the past 12 years. BNB will run to support MicroBooNE. Thought should be given as to what upgrades are desirable for an expanded short baseline neutrino program.

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Backup Slides

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Location

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MI12 (target location) 50 m absorber

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Beamline – Block Diagram

40 mr 42 m 80.5° bend 1.4 m dog-leg

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The Booster Neutrino Beamline was designed by Al Russel

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Beamline -- Schematic

Single Quadrupole Triplet Doublet Matching Permanent Magnets Final Focusing Triplet Carrier Pipe

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Optics

8 GeV. Designed to deliver 5E12 protons per pulse at 5 Hz average. ~40 degree phase advance per cell.

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Optics

Up to 12 m horizontal and 5 m vertical dispersion. Use large aperture (6-3-120) dipoles. Zero dispersion at target.

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Optics

  • Beam was bumped

upstream, both vertically and horizontally.

  • Quadruple transfer

functions were adjusted to match data.

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Optics

  • Known lattice functions at

851 are propagated down beamline.

  • Good match between

prediction and measurement. Changed momentum by inserting a piece of copper. Able to accurately predict perturbed trajectory.

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Keeping Beam on Target -- AutoTune

  • Change the current on a trim magnet and measure the movement on downstream BPMs:

∆ → ∆, ∆, ∆ ∆ → ∆, ∆

  • Leads to a linear equation:

∆ = ∆ ∆ ⋯ ∆ ∆ ⋮ ⋱ ⋮ ⋯ ∆ ∆

  • r

∆ = ∆

  • Choose correctors and BPMs so that “M” is invertible.
  • Can now solve for change in current given needed correction to positions:

∆ = ∆

  • To insure convergence:
  • Add tolerance to ideal position.
  • Make a fraction of the full correction.
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Modification

  • Added drainage tube

to return lines at five

  • ’clock and seven
  • ’clock position.
  • Minimizes stagnant

water.

  • Sept. 23, 2014

NBI2014 -- T. Kobilarcik 51

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Modification

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The target and horn are located in MI12B, accessed through the MI12 service building.

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Target/Horn in Target Pile

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Target Pile

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Well Pump

Transducer

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Three upstream wells Three downstream wells

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