1999 ATF Newsletters

March | April | May | June | July | August | Sept | Oct | Nov | Dec

May 14 | May 21 | May 28

 

Contents

1. Introduction

4. VISA
 
 

 

This week was a Mini-shutdown at the ATF and the NSLS Users Meeting.

Ilan Ben-Zvi.

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Experiments

 

Magnetic Measurements (Reported by George Rakowsky)

VISA: The pulsed wire bench has been reassembled on the smaller 12-ft granite table and measurements on Sections 1 and 2 have resumed. The new tabletops have come in from the shops. They have been mounted on the base pedestals in Bldg. 726 and are being surveyed and leveled. Robert Ruland’s interferomety rails have arrived from SLAC.

HGHG: Tilt limit switch hardware has been fabricated and is being installed on the Mini-undulator. In addition, limit switches are being installed on the ends of the magnet arrays to open on contact with the beampipe. Electronics modifications will be done next Tuesday.

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HGHG Experiment (Reported by Adnan Doyuran)

Yesterday the diving board has been installed, so I started aligning the He-Ne laser. Today I got the beam to the FEL room. The doubling crystal has been installed in front of the spectrometer. The crystal has a large wedge so it is tricky to align. Next week we will use the CO2 laser and try to generate 5 micron for the calibration of the spectrometer. Also I did another test about the detector. We were wondering how long this detector can operate after the cooling? I cooled about 1:30pm Thursday and measured the signal from a 5 micron diode. I got 63mV signal. I checked the signal frequently, lastly at 7:10pm I still measured 63 mV. Next day (Friday) at 11:30 am the signal was still 63 mV. I looked into the detector to check the liquid nitrogen level. It was cold, but no more liquid left. At 1:30pm the signal was gone totally. I cooled again and signal came back to 63 mV. I was surprised that after 22 hours signal was unchanged then in 2 hours it was gone. I checked the noise at about 1mV both when cold and warm.

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VISA Experiment Progress (Reported by Roger Carr)

Ben Poling and Roger Carr will arrive at BNL next Tuesday evening, and work next Wednesday, Thursday, and Friday to re-assemble VISA, with the newly machined pedestals and table tops. Marty Woodle informed me today that the table tops are not done as of today (Thursday), but he hoped that they would be done before Wednesday morning. He will informally QC them. We have sent all the ion pumps, the trim coil power supply buss, and all the small parts (washers, springs, etc) to BNL in preparation for our work next week. We hope to get the table tops mounted and aligned, and all the slides, bellows, etc remounted, fitted to the vacuum chambers, and to align the chambers. We have also designed and built a special jig for mounting the tungsten carbide kinematic mounts, and we will install them into the undulator modules.

If all goes well, the system will be ready for Robert Ruland and his crew to start work on mounting and aligning the modules, starting Monday, June 7. He expects that this work will take about 2 weeks. The beamline reference laser was shipped from UCLA to SLAC this week, where it will be checked out by Robert Ruland and crew.

During the period after undulator alignment, from June 21- July 6, the system is available for installation and checkout of optical and beam diagnostics, trim coils, vacuum systems, etc.

Any remaining design issues should be resolved by this time. If there is to be any kind of readiness review, it can occur in this period. Ben Poling and Roger Carr expect to return on July 6 to begin the move to ATF, and we hope to complete this work by July 16. If all goes well, Robert Ruland could begin the alignment in the ATF starting on July 19. However, if the schedule slips, and the system is not ready for him at this time, he will not be available again until September. Therefore, it is important that any delays be dealt with at high priority.

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VISA Beam and Radiation Probes (Reported by Erik Johnson)

We have our first pop-in probe of the new design to look at. Also this week

we received flippers that Alex ordered, the vacuum adapters, and the vacuum

actuators for the pop-ins. Some issues need still to be resolved for the

probe; the current mirror mount design was difficult (time consuming and

therefore expensive) to make, so an alternate is being explored for the

remaining probes. We also need to find out about how the mirror polishing

at UCLA is proceeding, and come up with an alternative way to get them

polished if it proves to be more difficult that first anticipated. The

attached file has a JPEG of the probe, one of the vacuum adapters, and one

of the actuators.

May_28_VISA_probe

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COMPTON Experiment Progress (Reported by Ping He and Shigeru Kashiwagi) Calibration of the silicon diode

We measured the number of generated electron hole pairs in the silicon diode using a 670nm, 10ns laser pulses. The capacitance of silicon diode was also measured using the special measurement system in Instrumentation division.

>From the capacitance measurement, the capacitance of diode is 329 pF at a

 

bias of 24V (220pF at biasVeV). Assume we use the silicon diode at 24V. The signal for 10^5 photons of 5 KeV (using 3.8 eV per electron-hole pair) is estimated at 0.0671 V.

The thickness of our silicon detector is estimated using the size (1" diameter) and capacitance of the silicon detector, taking the dielectric constant of silicon as 11.9:

~ 157 microns for C = 329 pF

~ 235 microns for C = 220 pF

 

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STELLA Experiment (Reported by Karl Kusche)

1) In preparation for the next scheduled run, various issues from the previous run were addressed. Included were camera iris and trim coil response, and the installation/alignment of a temporary pop-in inside of the ICA gas cell. This pop-in will allow us to better visualize the beam transport through the cell while the last triplet is oriented at 45 degrees. The results from the next run will help us to decide the final rotation angle of the triplet which will best compensate for the wiggler-induced skew.

2) The last portion of beamline #1 (between the cell and dipole) was reconnected, pumped out, and leak-checked. The entire beamline is now ready for the next run.

3) ICA optical system restoration & realignment continues in preparation for ICA recommissioning during the month of June.

4) The NSLS Safety Approval Form for STELLA was submitted for renewal, reflecting the recent changes in spectrometer shielding and internal gas cell configuration.

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STELLA Beam Optics (Reported by Ping He)

We have got an improved beam-optics result based on last version released May 14. The results are shown in the file at:

May_28_STELLA_Skew_optics

 

The results indicate that we have solved the problem of the skew quadrupole component in the IFEL wiggler.

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Facility

 

Computer Control System (Reported by Bob Malone)

1) Program for YAG energy feedback has been written. Debugging in progress.

2) New control system: 2/3 of network cabling have been installed.

 

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Technical Staff Tasks (reported by Bill Cahill)

Most of the week was spent trouble shooting the rf system, looking for the jitter that has plagued the ATF for over one week. Marc Montemagno found a deformed copper waveguide gasket on the reverse power terminator. The unit was repaired and the system appears very stable and noise levels have returned to acceptable levels. We recalibrated the time constant of the klystron water system to reduce the temperature recovery time. A power/sync chassis was built for the YAG camera system to further reduce the heat load on the table. Four YAG flash lamps needed replacement, two of which are done, the remaining will be changed over the weekend. Drawings were submitted for new mirror mounts to the NSLS Mechanical Group. Two mounts are currently being made, more to follow. The YAG amplifier chiller was relocated to the air conditioned "Z" line for improved temperature stabilization.

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CO2 Laser Status (Reported by Igor Pogorelsky)

Optics installed to deliver the alignment and amplified CO2 laser beams to the auto-correlator to measure the duration of the amplified pulse. Alignment of the auto-correlator setup is verified.

Mechanical work that permits delivery of the CO2 laser beam between the preamplifier, amplifier and experimental hall is completed. Installation of beam enclosures for the transport line is in progress. Work on eliminating gas leaks in the CO2 laser preamplifier and improving vacuum in the terawatt amplifier is in progress.

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Beam Studies (Reported by Vitaly Yakimenko)

The slow phase feed back system has been tested and the results are very satisfactory. The system uses the beam phase detector developed by Xijie Wang around the strip-line beam position monitor HSL4 (downstream of the linac). The results are shown in:

May_28__slow_phase_feedback

 

tm

One can see a correction of slow drift of up to 4 ps peak-to-peak over half an hour to essentially a non-measurable drift. The fast variations of about 1 ps are noise on the measurement system, not in the beam. This jitter is averaged out by the program to extract just the slow drift for correction.

Further testing is necessary to check for a correct behavior of the code for large phase jumps and verify that the phase stability of the detector does not introduce an error. This can be done by checking the energy stability on the high energy slits.

 

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Last Modified: December 3, 2007
Please forward all questions about this site to: Vitaly Yakimenko