ECR ion source for the highly charged intensive

  • Slides: 25
Download presentation
ECR ion source for the highly charged, intensive ion beams University of Jyväskylä, Department

ECR ion source for the highly charged, intensive ion beams University of Jyväskylä, Department of Physics H. Koivisto December 2007 ESF-Workshop, Athens, Greece

Content 1. Production of highly charged ion beams (by ECRIS) 2. Present projects and

Content 1. Production of highly charged ion beams (by ECRIS) 2. Present projects and challenges 3. (Metal) Ion beam production 4. Beam transport December 2007 ESF-Workshop, Athens, Greece

What kind of ion source? Accelerator (linear/cyclotron) gives some boundary condition! - Continues or

What kind of ion source? Accelerator (linear/cyclotron) gives some boundary condition! - Continues or pulsed beam? - A+ or Aq+(low versus high charge states)? - Intensity requirement? - Variety of elements? Charge breeding? Etc. . . ECRIS December 2007 ESF-Workshop, Athens, Greece

Operation principle (ECRIS) 1) Sufficient magnetic field (including correct structure) 2) Electrons rotating in

Operation principle (ECRIS) 1) Sufficient magnetic field (including correct structure) 2) Electrons rotating in magnetic field 3) Microwaves ECR: Electron Cyclotron Resonance December 2007 ESF-Workshop, Athens, Greece

Scaling laws (magnetic, frequency) 1) Magnetic field: Axial magnetic field Baxial by solenoids Radial

Scaling laws (magnetic, frequency) 1) Magnetic field: Axial magnetic field Baxial by solenoids Radial magnetic field Bradial by multipole 14 GHz : 0. 5 T 28 GHz: 1 T V E N U S December 2007 ESF-Workshop, Athens, Greece

Scaling laws 2) Frequency R. Geller proposed: as high microwave frequency as possible is

Scaling laws 2) Frequency R. Geller proposed: as high microwave frequency as possible is wanted! PROBLEM: Higher magnetic field is required!! December 2007 ESF-Workshop, Athens, Greece

ECRIS generations 1 st generation: 6. 4 GHz MSU RT-ECRIS, TAMU 6. 4 GHz,

ECRIS generations 1 st generation: 6. 4 GHz MSU RT-ECRIS, TAMU 6. 4 GHz, etc 2 nd generation: 14 GHz ECRIS AECR, Artemis, Caprice, etc. 3 rd generation: 28 GHz VENUS, SECRAL, several under construction: Requires SC-technique! December 2007 ESF-Workshop, Athens, Greece

The requirements of next generation heavy ion facilities made the development of 3 rd

The requirements of next generation heavy ion facilities made the development of 3 rd Generation sources (and maybe 4 th Generation) ECR ion sources necessary VENUS, 270 eµA U 33+ and 270 eµA U 34+ SC-ECRIS, RIKEN, Japan SECRAL, Lanzhou, China H. Zhao 525 eµA U 35+ MS ECRIS GSI, Germany December 2007 Su. SI NSCL, USA ESF-Workshop, Athens, Greece 50 -100 eµA U 41+ SPIRAL 2, GANIL, France 1 m. A Ar 12+

December 2007 ESF-Workshop, Athens, Greece

December 2007 ESF-Workshop, Athens, Greece

Optimization of the VENUS source for Ar 12+ to demonstrate the ‘tuning’ of the

Optimization of the VENUS source for Ar 12+ to demonstrate the ‘tuning’ of the plasma parameters Motivation: 1 m. A Ar 12+ for the SPIRAL II Project Ar VENUS (28 GHz) eμA December 2007 ESF-Workshop, Athens, Greece 12+ 860 14+ 514 16+ 270 17+ 36 18+ 1

Comparison of different generations 1 st generation: Itot<1 m. A ECRIS-56 2 nd generation:

Comparison of different generations 1 st generation: Itot<1 m. A ECRIS-56 2 nd generation: Itot= 2 -4 m. A Becr= 2 T 3 rd tot= 10 m. A Binjgeneration: I ~ 8 T Bext= 4 T Brad= 4 T Beyond present technological know-how! December 2007 ESF-Workshop, Athens, Greece

MS-ECRIS won’t be a 4 th generation ECRIS even if 56 GHz can be

MS-ECRIS won’t be a 4 th generation ECRIS even if 56 GHz can be tested It won’t fulfill the scaling law for the magnetic fields! It will be a step between the 3 rd and 4 th generation ECRIS (3. 5 generation) 4 th generation ECRIS requires a lot of development work for example in the field of superconductive technique December 2007 ESF-Workshop, Athens, Greece

Some engineering current densities December 2007 ESF-Workshop, Athens, Greece

Some engineering current densities December 2007 ESF-Workshop, Athens, Greece

Different Nb 3 Sn-structures Peak field December 2007 Solenoid 22 T Dipole 13 T

Different Nb 3 Sn-structures Peak field December 2007 Solenoid 22 T Dipole 13 T Quadrupole 10 T tested (4. 5 T pole) Sextupole + Solenoid Need ~14 T for 56 GHz ESF-Workshop, Athens, Greece

Cryostat and Cold Mass From Claude Lyneis Cryocooler Flange LN Reservoir (70 K) LHe

Cryostat and Cold Mass From Claude Lyneis Cryocooler Flange LN Reservoir (70 K) LHe Reservoir (4. 2 K) Vacuum Vessel 50 K Shield • Bremsstrahlung created in collisions of energetic electrons with the plasma chamber walls produce a high flux of x-rays. • A fair amount of this energy is deposited in the cryostat • With the original Al plasma chamber: Warm Bore Plasma Chamber • 1 W/k. W 28 GHz (only 2 W cooling power available) ass Cold M s Enclosed oil with C Links December 2007 Iron Yoke • 150 m. W/k. W for 18 GHz • High voltage insulation deteriorates in the high x-ray flux Bremsstrahlung will be a serious problem! ESF-Workshop, Athens, Greece

Challenges for 4 th generation ECRIS - superconducting wire to reach required B-field -

Challenges for 4 th generation ECRIS - superconducting wire to reach required B-field - bremsstrahlung (heating of cryostat) - cooling of plasma chamber (power up to tens of k. W) - coupling of microwaves to plasma - efficient extraction to handle multi tens of m. A beam December 2007 ESF-Workshop, Athens, Greece

Production of metal ion beams ECOS working group: “In order to meet the requirements

Production of metal ion beams ECOS working group: “In order to meet the requirements of the future experiments with high-intensity beams, further development is needed, especially in the production of metal-ion beams. Consequently, the development of ECR ion source will be one of the most active areas in accelerator physics. ” Consequently a lot of human resources will be invested in this work (very visible role during FP 7) December 2007 ESF-Workshop, Athens, Greece

Different methods: High temperature ovens: - inductively heated oven (above 2000˙C) December 2007 ESF-Workshop,

Different methods: High temperature ovens: - inductively heated oven (above 2000˙C) December 2007 ESF-Workshop, Athens, Greece

- resistively heated oven (above 2000˙C)) - sputtering (some refractory elements) - laser ablation?

- resistively heated oven (above 2000˙C)) - sputtering (some refractory elements) - laser ablation? December 2007 ESF-Workshop, Athens, Greece

Beam transport More beam intensity from the cyclotron is needed for the experiments!! Improvement

Beam transport More beam intensity from the cyclotron is needed for the experiments!! Improvement of ECRIS performance does not always increase the intensity for the experiments beam formation or/and transmission problem!! Problem in several laboratory! December 2007 ESF-Workshop, Athens, Greece

Statistics (2004) JYFL 14 GHz ECRIS Icycl/IECR 2 nd harmonic Transmission efficiency decreases when

Statistics (2004) JYFL 14 GHz ECRIS Icycl/IECR 2 nd harmonic Transmission efficiency decreases when beam intensity increases! Some reasons: 1) space charge effect (strong focusing) 2) Emittance increases with beam intensity December 2007 ESF-Workshop, Athens, Greece

DIMAD simulations (by X. Wu) Beam spot in viewer according to DIMAD-simulations Beam spot

DIMAD simulations (by X. Wu) Beam spot in viewer according to DIMAD-simulations Beam spot in viewer (just after dipole) December 2007 ESF-Workshop, Athens, Greece

Hollow beam JYFL NSCL December 2007 ESF-Workshop, Athens, Greece

Hollow beam JYFL NSCL December 2007 ESF-Workshop, Athens, Greece

“ECOS” needs the development of: - ion sources for higher intensity and higher charge

“ECOS” needs the development of: - ion sources for higher intensity and higher charge states - beam formation to produce high quality beams - high quality beam transport facility to transport beam efficiently to accelerator -development of metal ion beam production to make new and exotic beams available December 2007 ESF-Workshop, Athens, Greece

Thanks to the following for providing slides for this presentation: - Santo Gammino -

Thanks to the following for providing slides for this presentation: - Santo Gammino - Daniela Leitner - Claude Lyneis - Marc Doleans December 2007 ESF-Workshop, Athens, Greece