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T. Thuillier, CAS, Senec, 29/5-8/6 2012 CERN ACCELERATOR SCHOOL 2012: ELECTRON CYCLOTRON RESONANCE ION SOURCES - I Thomas Thuillier LPSC, 53 rue des Martyrs 38026 Grenoble cedex France E-mail: [email protected]

CERN ACCELERATOR SCHOOL 2012

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Page 1: CERN ACCELERATOR SCHOOL 2012

T. Thuillier, CAS, Senec, 29/5-8/6 2012

CERN ACCELERATOR SCHOOL 2012:

ELECTRON CYCLOTRON RESONANCE ION SOURCES - I Thomas Thuillier LPSC, 53 rue des Martyrs 38026 Grenoble cedex France E-mail: [email protected]

Page 2: CERN ACCELERATOR SCHOOL 2012

T. Thuillier, CERN Accelerator School 2012, Senec, 29/5-8/6 2012

OUTLINE

• Electron Cyclotron Resonance Ion Source - I •  Introduction •  Summary of the main microscopic processes occuring in an ECRIS •  Electron Cyclotron Resonance Mechanism •  Magnetic confinement and ECR plasma generation •  Geller Scaling Law and ECRIS Standard Model

CAS 2012 – ECR Ion Sources I

2

Page 3: CERN ACCELERATOR SCHOOL 2012

T. Thuillier, CERN Accelerator School 2012, Senec, 29/5-8/6 2012

Ingredients of Electron Cyclotron Resonance Ion Source •  An ECR ion source requires:

•  A secondary vacuum level to allow multicharged ion production •  A RF injection in a metallic cavity (usually multimode) •  A sophisticated magnetic Field structure that enables to:

•  Transfer RF power to electrons through the ECR mechanism •  Confine long enough the (hot) electrons to ionize atoms •  Confine long enough ions to allow multi-ionization ions •  Generate a stable CW plasma

•  An atom injection system (gas or condensables) to sustain the plasma density •  An extraction system to accelerate ions from the plasma

•  In the following, we will try to detail these points to provide an overview of ECR ion sources

3

Extracted Ion beam

Wall

vacuum

Atoms

RF power Magnetic Field lines

ECR ZONE

ECR PLASMA

Introduction

Page 4: CERN ACCELERATOR SCHOOL 2012

T. Thuillier, CERN Accelerator School 2012, Senec, 29/5-8/6 2012

Ion creation through Electron Impact Ionization (in gas or plasma) • 

4

In

2-3×In

Electron kinetic Energy

High energy tail

Elec

tron

Im

pact

Cro

ss s

ecti

on

Summary of the main microscopic processes occuring in an ECR Ion Source

Page 5: CERN ACCELERATOR SCHOOL 2012

T. Thuillier, CERN Accelerator School 2012, Senec, 29/5-8/6 2012

Ion creation through Electron Impact Ionization (in gas or plasma)

• 

5

In= nth Ionization Potential

Z In (eV)

1+ 7.2 ~2.4×10-16

22+ 159 ~4.9×10-19

54+ 939 ~1.4×10-20

72+ 3999 ~7.8×10-22

82+ 90526 ~1.5×10-24

Example for Bismuth

Bi

Summary of the main microscopic processes occuring in an ECR Ion Source

Page 6: CERN ACCELERATOR SCHOOL 2012

T. Thuillier, CERN Accelerator School 2012, Senec, 29/5-8/6 2012

Ion loss through Charge-Exchange (in gas or plasma) • 

6

Z 1+ 22+ 54+ 72+ 82+

1.5×10-15 5.6×10-14 1.6×10-13 2.2×10-13 2.6×10-13

Example : Bismuth with O2

Summary of the main microscopic processes occuring in an ECR Ion Source

Page 7: CERN ACCELERATOR SCHOOL 2012

T. Thuillier, CERN Accelerator School 2012, Senec, 29/5-8/6 2012

Zero Dimension Modelization • 

7

Summary of the main microscopic processes occuring in an ECR Ion Source

creation destruction

Losses (ion extraction,

wall…)

Page 8: CERN ACCELERATOR SCHOOL 2012

T. Thuillier, CERN Accelerator School 2012, Senec, 29/5-8/6 2012

Elastic Collision in an ECRIS plasma • 

8

Summary of the main microscopic processes occuring in an ECR Ion Source

90°

Page 9: CERN ACCELERATOR SCHOOL 2012

T. Thuillier, CERN Accelerator School 2012, Senec, 29/5-8/6 2012

Motion of a charged particle in a constant magnetic field • 

9

Electron Cyclotron Resonance Mechanism

Page 10: CERN ACCELERATOR SCHOOL 2012

T. Thuillier, CERN Accelerator School 2012, Senec, 29/5-8/6 2012

The Electron Cyclotron Resonance (1/3) • 

10

Electron Cyclotron Resonance Mechanism

Page 11: CERN ACCELERATOR SCHOOL 2012

T. Thuillier, CERN Accelerator School 2012, Senec, 29/5-8/6 2012

The Electron Cyclotron Resonance (2/3) • 

11

e- Electron trajectory

Electron Cyclotron Resonance Mechanism

Page 12: CERN ACCELERATOR SCHOOL 2012

T. Thuillier, CERN Accelerator School 2012, Senec, 29/5-8/6 2012

The Electron Cyclotron Resonance (3/3) • 

12

ECR Heating here

Electron Cyclotron Resonance Mechanism

Page 13: CERN ACCELERATOR SCHOOL 2012

T. Thuillier, CERN Accelerator School 2012, Senec, 29/5-8/6 2012

ECR Stochastic Heating (1/5) • 

13

Electron accelerates

Electron decelerates!

Electron Cyclotron Resonance Mechanism

Page 14: CERN ACCELERATOR SCHOOL 2012

T. Thuillier, CERN Accelerator School 2012, Senec, 29/5-8/6 2012

ECR Stochastic Heating (2/5) • 

14

Former solution (v0=0)

Initial condition (v0≠0)

Electron Cyclotron Resonance Mechanism

Page 15: CERN ACCELERATOR SCHOOL 2012

T. Thuillier, CERN Accelerator School 2012, Senec, 29/5-8/6 2012

ECR Stochastic Heating (3/5) • 

15

Constant term

Electron Cyclotron Resonance Mechanism

Page 16: CERN ACCELERATOR SCHOOL 2012

T. Thuillier, CERN Accelerator School 2012, Senec, 29/5-8/6 2012

ECR Stochastic Heating (4/5) • 

16

HEATING

COOLING!

Electron Cyclotron Resonance Mechanism

Page 17: CERN ACCELERATOR SCHOOL 2012

T. Thuillier, CERN Accelerator School 2012, Senec, 29/5-8/6 2012

ECR Stochastic Heating (5/5) • 

17

Electron Cyclotron Resonance Mechanism

Page 18: CERN ACCELERATOR SCHOOL 2012

T. Thuillier, CERN Accelerator School 2012, Senec, 29/5-8/6 2012

ECR Heating in a Magnetic Gradient • 

18

z

B(z) ECR

Heating zone

BECR

Electron Cyclotron Resonance Mechanism

Page 19: CERN ACCELERATOR SCHOOL 2012

T. Thuillier, CERN Accelerator School 2012, Senec, 29/5-8/6 2012

Properties of particle motion in a magnetic field (1/2) • 

19

Magnetic Field line In a Tokamak

http://www-fusion-magnetique.cea.fr

Magnetic Confinement and ECR Plasma Generation

Page 20: CERN ACCELERATOR SCHOOL 2012

T. Thuillier, CERN Accelerator School 2012, Senec, 29/5-8/6 2012

Properties of particle motion in a magnetic field (2/2) • 

20

Magnetic Confinement and ECR Plasma Generation

Page 21: CERN ACCELERATOR SCHOOL 2012

T. Thuillier, CERN Accelerator School 2012, Senec, 29/5-8/6 2012

The Magnetic Mirror Effect • 

21

Axial mirror done with a set of 2 coils

http://www.astronomes.com/

Solar wind reflection by the

Earth magnetosphere

Magnetic Confinement and ECR Plasma Generation

Page 22: CERN ACCELERATOR SCHOOL 2012

T. Thuillier, CERN Accelerator School 2012, Senec, 29/5-8/6 2012

Corrolary of Magnetic Mirroring: The Loss Cone • 

22

VII

V┴

θmin confined Particles

Loss cone

In an ECRIS plasma, The loss cone is perpetually populated By particles interaction (Spitzer)

Magnetic Confinement and ECR Plasma Generation

Page 23: CERN ACCELERATOR SCHOOL 2012

T. Thuillier, CERN Accelerator School 2012, Senec, 29/5-8/6 2012

ECR Magnetic confinement: Minimum |B| structure • ECR ion sources features a sophisticated magnetic field

structure to optimize charged particle trapping •  Superimposition of axial coils and hexapole coils •  The ECR surface (|B|=BECR) is closed

23

Iso B lines

z

Bz Axial Mirror

BECR

BECR

Source LBNL

Hexapolar Field

Source RIKEN, Nakagawa

|B|(x,z)

z 2r Source D. Xie

Magnetic Confinement and ECR Plasma Generation

Page 24: CERN ACCELERATOR SCHOOL 2012

T. Thuillier, CERN Accelerator School 2012, Senec, 29/5-8/6 2012

Axial Magnetic Confinement • The axial magnetic confinement in a

multicharged ECRIS is usually done with a set of 2 or 3 axial coils. •  Either room temperature coils + iron to

boost the magnetic field •  Or superconducting coils

•  In the case of 3 coils, the current intensity in the middle one is opposed to the others so that it helps digging Bmed

• Usually Binj, Bext respectively stand for the magnetic field at injection (of RF, atoms…) and (beam) extraction

• Bext should be the smaller magnetic field in the ECR to favor Ion extraction there!

24

z

Bz

Axial Mirror

Binj

Bmed

Bext

z

cinj

cmed cext

r

Magnetic Confinement and ECR Plasma Generation

Page 25: CERN ACCELERATOR SCHOOL 2012

T. Thuillier, CERN Accelerator School 2012, Senec, 29/5-8/6 2012

Radial Magnetic Confinement • The radial magnetic confinement

is usually built with a hexapole field

• Either with permanent magnets •  Br Up to 1.6 T maximum possibly 2T

with some tricks •  Advantage : economical •  Inconvenient: not tunable

• Either with a set of superconducting coils •  Br>1.6 T-2 T •  Advantage: tunable online to

optimize a population of ion in the source.

•  Inconvenient: expensive, complicated design and building

25

|Br|

r

(HallBach Hexapole With 36 permanent magnets

30° rotation/magnet)

r

Superconducting hexapolar coil

Magnetic Confinement and ECR Plasma Generation

Page 26: CERN ACCELERATOR SCHOOL 2012

T. Thuillier, CERN Accelerator School 2012, Senec, 29/5-8/6 2012

ECR Plasma build up

• 

26

vacuum Atoms

RF

Extraction

Magnetic Confinement and ECR Plasma Generation

Page 27: CERN ACCELERATOR SCHOOL 2012

T. Thuillier, CERN Accelerator School 2012, Senec, 29/5-8/6 2012

The Famous plasma shape in an ECR Ion Source • To understand why the ECR plasma ends with 3 lines only, one

needs to follow the heated electron through the ECR zone

27

Br

Bz

Near to the wall

Near to the axis: axial field only

HOT ECR ELECTRONS ⇒ High density Plasma ⇒ LIGHT emission ⇒ Tracks on walls

No hot electrons ⇒ Low density Plasma ⇒ No Light emission ⇒ No Tracks on walls

Plasma shape at injection (L) and Extraction (R)

Half unrolled Liner with plasma marks (3 poles= π only)

z

Photo of ECR plasma from injection (all thickness is superimoosed=> 6 lines) 10+14 GHz heating

Elevation view from an ECRIS chamber along 2 hexapole poles

Magnetic Confinement and ECR Plasma Generation

Page 28: CERN ACCELERATOR SCHOOL 2012

T. Thuillier, CERN Accelerator School 2012, Senec, 29/5-8/6 2012

Plasma Oscillations – ECR cut off density • 

28

Geller Scaling Law and ECRIS Standard Model

Above cut off: RF is reflected => no more ECR heating!

Page 29: CERN ACCELERATOR SCHOOL 2012

T. Thuillier, CERN Accelerator School 2012, Senec, 29/5-8/6 2012

The ECR Scaling law (R. Geller, 1987) • 

29

fECR

[GHz] λECR [cm]

ne

[cm-3] Λ0->1+

[cm] τ0->1+

[µs] B

ECR [T]

2.45 ~12 7.4 ×1010 ~7 ~10 0.09

14 ~2 2.5×1012 0.2 3 0.5

28 ~1 ~1013 0.05 0.7 1

60 ~ 0.5 4.4×1013 0.01 0.17 2

Geller Scaling Law and ECRIS Standard Model

Page 30: CERN ACCELERATOR SCHOOL 2012

T. Thuillier, CERN Accelerator School 2012, Senec, 29/5-8/6 2012

The ECR standard model • Optimum high charge state ion production and extraction have been

experimentally studied as a function of ECR frequency. • General Scaling laws for the magnetic field have been established

30

r

Br

Binj

Bmed

Bext

Axial Mirror Radial Mirror

~1990 2003 ?

fECR [GHz] 14 28 56

BECR [T] 0.5 1 2

Brad~2×BECR 1 2 4

Binj~3-4×BECR 2 3.5 7

Bmed~0.5-0.8×BECR 0.25 0.5 1

Bext≤Brad 1 2 4

VENUS

|B|(x,z)

z 2r Source D. Xie

Z

Geller Scaling Law and ECRIS Standard Model