Courtney Knaup Emporia State University REU 2007 Cyclotron Institute, Texas A&M University Advisor: Dr. Henry Clark Upon completion of the recommissioning.

Slides:



Advertisements
Similar presentations
Applications of the Motion of Charged Particles in a Magnetic Field AP Physics C Montwood High School R. Casao.
Advertisements

The Front End Test Stand Collaboration ELECTROMAGNETIC DESIGN OF A RFQ FOR THE FRONT END TEST STAND AT RAL A. Kurup, A. Letchford The RAL front end test.
Chapter 29 Magnetic Fields.
ILC Accelerator School Kyungpook National University
Bastille Day 2000 Solar Energetic Particles Event: Ulysses observations at high heliographic latitudes M. Zhang Florida Institute of Technology.
An Advanced Linear Accelerator Facility for Microelectronic Dose Rate Studies P.E. Sokol and S.Y.Lee Indiana University.
Hall D Photon Beam Simulation and Rates Part 1: photon beam line Part 2: tagger Richard Jones, University of Connecticut Hall D Beam Line and Tagger Review.
Status of the Tagger Hall Background Simulation Simulation A. Somov, Jefferson Lab Hall-D Collaboration Meeting, University of Regina September
Using Tune Shifts to Evaluate Electron Cloud Effects on Beam Dynamics at CesrTA Jennifer Chu Mentors: Dr. David Kreinick and Dr. Gerry Dugan 8/11/2011REU.
Sub-THz Component of Large Solar Flares Emily Ulanski December 9, 2008 Plasma Physics and Magnetohydrodynamics.
Magnetic Field and Magnetic Forces
Searching for CesrTA guide field nonlinearities in beam position spectra Laurel Hales Mike Billing Mark Palmer.
Danish Space Research Institute Danish Small Satellite Programme FH Space_Environment.ppt Slide # 1 Flemming Hansen MScEE, PhD Technology Manager.
Triangle Universities Nuclear Laboratory July 26, 2001-TUNL REU The Making and Using of Spin-Polarized H  and D  Beams.
TJR 7/30/031 Geant4 Simulations of the MICE Beamline Tom Roberts Illinois Institute of Technology 7/30/03.
Super-B Factory Workshop January 19-22, 2004 Super-B IR design M. Sullivan 1 Interaction Region Design for a Super-B Factory M. Sullivan for the Super-B.
Henry L. Clark, Ph D Accelerator Physicist / SEE Line Project Manager / Upgrade Project Manager Cyclotron Institute, Texas A&M University.
BROOKHAVEN SCIENCE ASSOCIATES Abstract Magnetic Specifications and Tolerances Weiming Guo, NSLS-II Project In this presentation I briefly introduced the.
SMURF Research at Texas A&M
1 Light Collection  Once light is produced in a scintillator it must collected, transported, and coupled to some device that can convert it into an electrical.
FAA/NASA Joint University Program for Air Transportation Research Jeff Dickman Chris Bartone June 20, 2003 A New Anechoic Chamber for Nearfield Antenna.
Applications of Particle Deflection Lesson 4. Objectives explain, quantitatively, how uniform magnetic and electric fields affect a moving electric charge,
NEEP 541 Radiation Interactions Fall 2003 Jake Blanchard.
Physics of Particle Accelerators Kalanand Mishra Department of Physics University of Cincinnati.
P. Scampoli - 24th ICNTS Bologna, September 4,
Tools for Nuclear & Particle Physics Experimental Background.
Jornadas LIP 2008 – Pedro Ramalhete. 17 m hadron absorber vertex region 8 MWPCs 4 trigger hodoscopes toroidal magnet dipole magnet hadron absorber targets.
The ISIS strong focusing synchrotron also at the Rutherford Appleton Laboratory. Note that ISIS occupies the same hall as NIMROD used to and re- uses some.
Mass Spectroscopy 1 Mass Spectroscopy (Mass Spec) Applying Atomic Structure Knowledge to Chemical Analysis.
Summer Practice in JINR Mathematical modeling of high-energy particle beams in accelerators.
Proposal for Experiment S291: " Residual radioactivity induced by U ions - experimental investigation and longtime predictions" GSI, Darmstadt: G.Fehrenbacher,
In this experiment, C 60 was photoionized with single photons with specified energies between the energy range of 37 to 160eV. The photons used came from.
Alpha and Beta Interactions
Space Environment SSE-120 Please type in your questions and raise your hand so we can answer it during class.
Radiation damage calculation in PHITS
Magnetic Fields. Definition : A magnetic field is a force field which surrounds either a magnet or a wire carrying an electric current and will act upon,
Chapter 28 Lecture 26 Magnetic Fields: I. Magnetic Poles Every magnet, regardless of its shape, has two poles Called north and south poles Poles exert.
1 BROOKHAVEN SCIENCE ASSOCIATES NSLS-II Overview Satoshi Ozaki Director, Accelerator Systems Division NSLS-II Project March 27, 2007.
Magnetic Field and Magnetic Forces
Experiment Electronics UMC 0.18µm radiation hardness studies Progress since last Collaboration Meeting Sven Löchner GSI Darmstadt 15 th CBM Collaboration.
MBA Magnets MultiBend Achromat Magnets 8/14/2015 Review By Mark Jaski.
FCC-hh: First simulations of electron cloud build-up L. Mether, G. Iadarola, G. Rumolo FCC Design meeting.
By: Paul Lim and Brittany Griner.  Reliable, radiation resistance, and spin stabilized  Approximately 370kg (814 pounds)  Box-like main structure 1.65.
© 2003 By Default! A Free sample background from Slide 1 JINR SCIENTIFIC COUNCIL 102 nd Session, September 2007, Dubna.
Present status of production target and Room design Takashi Hashimoto, IBS/RISP 2015, February.
Experimental Cave at Trento CPT: status update Francesco Tommasino RDH/IRPT Meeting – Roma, 1 Feb 2016.
Paul Scherrer Institut 5232 Villigen PSI EURISOL/BENE_2007, PSI /GF34 Joint High Power Target Meeting EURISOL/BENE , CERN Direct target irradiation.
Ion Accelerator Activities at VECC
Halo Collimation of Protons and Heavy Ions in SIS-100.
Applications of Particle Deflection
Polyimide sheet (5 mils)) AZ-93 Thermal Paint (5 mils))
The BLAIRR Irradiation Facility Hybrid Spallation Target Optimization
Update to ECLOUD Calculations for the
Chapter 4 Antenna Arrays
Standaert Laurent UCL- Cyclotron Resource Centre
Options and Recommendations for TL and Dumps
ARTEMIS – solar wind/ shocks
Arc magnet designs Attilio Milanese 13 Oct. 2016
On the ARIEL Pre-separator
Thermal emittance measurement Gun Spectrometer
Chapter 3, Part3 Nuclear Chemistry CHEM 396 by Dr
Figure 20.1  Joule’s experiment for determining the mechanical equivalent of heat. The falling blocks rotate the paddles, causing the temperature of the.
Figure 20.1  Joule’s experiment for determining the mechanical equivalent of heat. The falling blocks rotate the paddles, causing the temperature of the.
Interaction Region Design Options e+e- Factories Workshop
Chapter 29 Problems Problems 7, 9, 12, 30, 37, 41.
Beam Loss Simulations LHC
ICRC2003 OG Calculation of Cosmic-Ray Proton and Anti-proton Spatial Distribution in Magnetosphere Michio Fuki, Ayako Kuwahara, Nozomi, Sawada Faculty.
B.Sc.II, Paper VIII ( IIISemester)
5/3/2019 Magnetic Forces, Materials, and Devices 1.
MEIC Shifting Magnet Tim Michalski August 6, 2015.
Presentation transcript:

Courtney Knaup Emporia State University REU 2007 Cyclotron Institute, Texas A&M University Advisor: Dr. Henry Clark Upon completion of the recommissioning project, the Cyclotron Institute can expand the Radiation Effects Facility (REF) program by adding a dedicated beam line and experimental cave on the K150 cyclotron. The beam line layout, testing station and radiation shielding walls have been designed. The computer code “Transport” was used to determine the number of electromagnets needed and their optimal positions along the beam line so that both defuse and focused beam spots can be produced at the target location. A list of ions at energies produced by the K150 cyclotron has been determined for the Single Event Effects (SEE) experimenters. The SEE experimenters require a wide variety of ions and energies in order to effectively test their computer chips. The curve in the figure above shows the maximum E/A as a function of Q/M for the K150 cyclotron. To reduce tuning time between ion changes, sets of ions at similar Q/M ratios have been determined. The design of the experimental area allows plenty of room for work space, radiation shielding, and an entrance labyrinth which allows for easy access and the containment of secondary radiation produced by the beam. Due to space limitations, an "all in one" in-air/vacuum chamber testing station has been re-designed. The K500 REF beam line uses two separate areas; one for in-air testing and one for vacuum testing. the new design allows the beam line to be much shorter while not compromising its usefulness. Beam is transported along the beam line from the K150 cyclotron. The quadrupole magnet pairs focus and/or defocus the beam and the dipole magnet bends the beam into the experimental area. The computer code “Transport” was used to determine the optimal positions for quadrupole magnet pairs 2, 3 and 4. The magnetic fields of the quadrupole magnet pairs can be set so that the beam spot at the testing station is either diffuse or focused. The diagrams above show the phase space of the beam along the beam path for a diffuse beam spot scenario. This structure is required for the SEE experiments and ensures that their computer chips are uniformly irradiated. Computer chips in aerospace equipment receive high levels of radiation from solar flares, cosmic rays and the Earth's Van Allen radiation belts. The performance of these chips can be tested with the accelerated beams from the K150 cyclotron which are similar in ion type and close to the energies experienced in space. Aerospace engineers plot the number of upsets as a function of LET to understand how well their computer chips will respond in the radiation fields of the earth. Upset cross sections tend to follow the pattern shown in the figure above which includes three parts: the threshold, knee and saturation regions. With ions having range of ~100 microns and LET up to ~60 MeV/mg/cm2, engineers can test "In-air" and up to LETs into the saturation region with the K150 accelerated beams. The charts above show the linear energy transfer (LET) as a function of range for ions accelerated to 5, 14, and 25A MeV/nucleon. The 14 and 25 MeV/nucleon ions have enough energy to allow experimenters to test in air.