ECR Plasma Physics and Production of Highly Charged … · T=0.5 mA I T=2-4 mA I T > 5 mA I ......

52
18 th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 1 Santo Gammino Istituto Nazionale di Fisica Nucleare LABORATORI NAZIONALI DEL SUD S. Gammino for the ISIBHI collaboration INFN - GSI - GANIL - CEA - JYFL - KVI - TSL - CERN - NIPNE - IKF ECR Plasma Physics and Production of Highly Charged Heavy Ion from MS-ECRIS

Transcript of ECR Plasma Physics and Production of Highly Charged … · T=0.5 mA I T=2-4 mA I T > 5 mA I ......

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 1Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

S. Gammino for the ISIBHI collaboration

INFN - GSI - GANIL - CEA - JYFL - KVI - TSL - CERN - NIPNE - IKF

ECR Plasma Physics and Production of HighlyCharged Heavy Ion from MS-ECRIS

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 2Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

Outline

1. The ECR laws and their limits: experimental evidences.

2. The 3rd generation ECRISs and the status of the MS-ECRIS

source.

3. Possible future steps with MS-ECRIS and beyond.

4. Warning: usually invited speakers give answers, I will often pose

questions…

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 3Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

Intense beams of highly charged heavy ions

• Intense beams: study of rare processes (RIBs, SHE).

• Highly charged ions -->> higher energy for

cyclotron beams.

• Heavy ions (particularly metals) are needed.

• These requests may be fulfilled by 3rd generation

ECRIS (f > 24 GHz, B > 3 T).

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 4Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

1st generation

2nd generation

3rd generation

(killed)othersgood & bad

2 . 5generation

ECRIS generations(presented at HIAT’98)

IT=0.5 mA

IT=2-4 mA

IT > 5 mA

IT >10 mA

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 5Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

How to increasehighly charged ion production?

• Up to recent times, the continuous improvements of magnettechnology and RF generators technology have guided the stepstowards the use of higher magnetic field and higher microwavefrequency to heat the electrons via the ECR heating.

• A simple scaling of frequency and magnetic field according to the Geller’s scaling laws cannot be continued ‘ad libitum’ as we are nearthe limit of magnets’ technology.

• Additional limitation: ECR plasma physics is not completelyunderstood.

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 6Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

a) the radial magnetic field value at the plasma chamber wall must be Brad

≥ 2 BECR;

b) the axial magnetic field value at

injection must be about Binj ≈3BECR or more;

c) the axial magnetic field value at

extraction must be about Bext ≈ Brad ;

d) the axial magnetic field value at the minimum must be in the range 0.30 < Bmin/Brad<0.45.

Topt (eV)

neτi

(cm-3

sec)

He 2+

Ar 18+

Li3+

Be4+

B5+

C6+

N7+

O8+Ne10+

Si14+

Fe25+

Kr36+

Xe54+

U92+

2nd generationECRIS

4th generationECRIS

3rd generationECRIS

(U6+,Xe6+ ,Kr 6+ ,Ar5+ ,Ne 4+ ,N3+)

(U12+ ,Xe 12+ ,Kr11+ ,Ar7+,Ne6+,N4+)

(U24+ ,Xe20+ ,Kr17+ ,Ar11+ ,Ne7+ ,N5+)

(U28+ ,Xe21+ ,Kr18+ ,Ar12+ ,Ne8+ ,N6+)

(U34+ ,Xe23+ ,Kr20+ ,Ar14+ ,Ne9+)

(U 47+ ,Xe35+ ,Kr26+ ,Ar16+)

(U55+ ,Xe40+ ,Kr29+ ,Ar17+)

(U 64+ ,Xe44+ ,Kr32+)

(U76+ ,Xe48+ ,Kr34+ )

(U 90+ )

(U 82+ ,Xe52+ )

Topt (eV)

neτi

(cm-3

sec)

He 2+

Ar 18+

Li3+

Be4+

B5+

C6+

N7+

O8+Ne10+

Si14+

Fe25+

Kr36+

Xe54+

U92+

2nd generationECRIS

4th generationECRIS

3rd generationECRIS

(U6+,Xe6+ ,Kr 6+ ,Ar5+ ,Ne 4+ ,N3+)

(U12+ ,Xe 12+ ,Kr11+ ,Ar7+,Ne6+,N4+)

(U24+ ,Xe20+ ,Kr17+ ,Ar11+ ,Ne7+ ,N5+)

(U28+ ,Xe21+ ,Kr18+ ,Ar12+ ,Ne8+ ,N6+)

(U34+ ,Xe23+ ,Kr20+ ,Ar14+ ,Ne9+)

(U 47+ ,Xe35+ ,Kr26+ ,Ar16+)

(U55+ ,Xe40+ ,Kr29+ ,Ar17+)

(U 64+ ,Xe44+ ,Kr32+)

(U76+ ,Xe48+ ,Kr34+ )

(U 90+ )

(U 82+ ,Xe52+ )

qopt ∝ log B3/2

Iq+ ∝ f2 Mi- 1

Scaling laws, High B mode, Golovanivsky plot

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 7Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

If we consider a simple scaling law for the magnetic field and frequency, we

obtain 3-5 T for the 3rd generation ECRIS and 28-37 GHz operational

frequency; 6-8 T for the 4th generation and 56-75 GHz frequency.

The former case is still within the existing technology of

magnets and RF generators.The latter case it is not for the magnets, as these field can be

obtained only with Nb3Sn magnets, but maybe it will be in the next decade (progresses are ongoing).

Scaling to 3rd and 4th generationECRIS

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 8Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

It is not also for microwave generators, as a generator of the right frequency (40 to 60 GHz) and power (in the range of tens of kW), working in cw mode, has to be built ‘ad hoc’.

Power is a major issue, in fact following a simple scaling laws

P = V Ee ne/τe

for a 4th generation ECRIS we would need more than 50 kW !

Microwave power

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 9Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

For MS-ECRIS and for the next generation of ECR sources it will be

necessary to master critical issues of plasma physicsmaster critical issues of plasma physics to fully exploit

their characteristics.

Even if relevant technological achievement may provide higher

confining field and higher power/frequency microwave generators,

they will be not useful without the competent understanding of non-

linear effects arising in the ECRIS plasma.

These considerations are reinforced by experimental results:

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 10Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

Some experimental ‘strange’ data

0

20

40

60

80

100

1 1,2 1,4 1,6 1,8 2 2,2 2,4 2,6 2,8 3

Brad / B res

Inte

nsity

(eµA

)

28 GHz18 GHz14 GHz

Xe27+

SERSEAug-Sept. 2000

SERSE Oct. 2001-summer 2002

0

10

20

30

40

50

60

70

80

90

0 100 200 300 400 500 600 700 800

Power [W]

Cur

rent

[eµA

]

KLY-18TWT1-18

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 11Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

There is something exceptHBM and scaling laws

• The explanation was found in the assumption that

microwaves injection and coupling to the plasma as well

as ECR heating is not a simple matter of ‘brute force’ but

the way that microwaves are injected is important.

• L. Celona proposed different schemes of microwaves

injection at ECRIS’04 workshop at LBNL.

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 12Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

Broadband generators and ECR condition

When TWT is used VOLUME EFFECT takes place?

∆+=

∆−=

)(2

)(2

2

1

υυπ

υυπ

EMe

e

EMe

e

qmB

qmB e-

Volume ECR conditions

B2

B1

EMe

eECR q

mBB υπ2==

e-

Standard ECR conditions

BECR

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 13Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

•SERSE test with broad frequency spectrum(continuous and discrete)

•White noise generator

•Test with a passband filter (able to withstand the full power of the microwave generator) to select exactlythe needed bandwidth.

•Accurate modelling of the phenomena.

•Development of broadband microwave generator (e.g. GyroTWT) is requested.

From the talk given by L.Celonaat ECRIS’04

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 14Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

The explanation in terms of a broader resonance related to the broad bandwidth of the amplifier was not fully convincing: itdoes not explain the different results when different sourcesoperate in Two Frequency Heating mode.

An experiment with White Noise Generator, was successfullycarried out by a JYFL-ORNL collaboration in 2005 (Y. Kawaiet al, Rev.Sci.Instr. 77,03A331).

An improvement of a factor 2-3 was obtained for the current of the highest charge states produced by a old 6.4 GHz ECRIS (the amount of power was only about 200 W).

Broader resonance or something else?

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 15Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

In the meantime the need to define the ideal position of the waveguide

ports in MS-ECRIS made necessary to study the shape of modes excited

inside the plasma chamber; a parallel study about the effectiveness of the

ECR heating in the case of the SERSE source made clear that the

important figure is not the maximum field in the plasma chamber but the

maximum value that the field reaches on the resonant surface.

Some experimental results made this picture more convincing, showing

that minor changes of frequency may be relevant on the performance as

they rapidly and completely change the maximum of the field.

Frequency tuning effect

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 16Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

CAPRICE -GSIfall 2006

L. Celona et al.

SUPERNANOGAN - CNAO July 2005

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 17Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

Are we able to apply these resultsto existing ECRIS?

• Different sources use TWT generator and alreadyoperate the frequency tuning.

• 14 and 18 GHz Klystron generators may be also tunedwithin few tens of MHz.

• Gyrotrons cannot, but microwave launching and modesexcitation in the plasma chamber may be optimized(latest point is still to be studied).

• Minor investment may take to relevant performance increase (multi-frequency heating is still not fullyexploited).

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 18Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

Simulatedelectron

distribution

LossCone

NO e.m. field

Simulations’ Results forSingle Frequency Heating

The e.m. field allows to confine up to

60% of electrons that otherwise go away from the plasma.

Resonance surface

e.m. wave @ 1000 W

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 19Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

Improvement of the electron heatingby means of Two Frequency Heating - TFH

plasma heating with two electromagnetic wavesinstead of one, by using two lower power values

Strong ECR plug effectand plug-in

Energy Saturation at higher powers

possibility to optimize the plasma heating by efficient transfer of the electromagnetic energy

ECR Zone in a minimum-B

magnetic field

e- e-I ECR Zone

II ECR Zone

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 20Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

ECR Heating dependence on the electromagnetic field shape

The electron heating occursonly in the resonance region

14 GHz – TE4,4,23 mode 18 GHz – TE4,6,22 modeFor TE4,4,23 the electric field is five times higher than TE4,6,22 at the resonance

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 21Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 22Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

How to apply these resultsto 3rd generation ECRIS?

• Microwave launching and modes excitation in the plasma

chamber may be optimized.

• The magnetic field parameters are to be adapted to the

microwave field distribution.

• For TFH a TWT generator should be used in order to

operate the frequency tuning.

• Broadband high frequency generator should be built (above

28 GHz), not necessarily above 10 kW.

• Further insights in the ECR plasma physics is mandatory to

fully exploit 3rd generation ECRISs.

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 23Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

II part

• State of the art of 3rd generation ECRIS

• The MS-ECRIS source

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 24Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

VENUS @ LBNL

VENUS

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 25Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

Inject. Solenoid

Middle Solenoid

Extract. Solenoid

Sextupole Coil

Aluminum Clamping Ring

Iron Segments for SextupoleField Booster and coil Clamping

Iron York and Shielding

Iron pole

SECRAL(IMP, Lanzhou, China)

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 26Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

SuSISuSI @ NSCL@ NSCLSuperconducting Source for IonsSuperconducting Source for Ions

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 27Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

60 kV extraction

voltage

HTS CoilsUHV seals

Large permanent magnet hexapole

Copper CoilLateral hexapole

A-PHOENIXa hybrid ECR Ion Source

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 28Santo Gammino

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RIKEN SCRIKEN SC--ECRIS(28GHz)ECRIS(28GHz)

Goal for RIBF15 pµA of U35+

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 29Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

VENUS

Bradial 2.1 TBaxial 4.0 TVext 20 kV

φ chamber 150 mm

SECRAL

2 T3.6 T

20-30 kV126 mm

A-PHOENIX

1.7-2.2 T3 T

60 kV70 mm

SuSI

2.0 T3.6 T60 kV

100 mm

MS-ECRIS

2.7 T4.5 T

40-60 kV180 mm

RIKEN

2 T4 T---

150 mm

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 30Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

Multipurpose Fully SuperconductingMagnets ECRIS (MS-ECRIS)

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 31Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

ISIBHI collaboration

• EU has partially funded the MS-ECRIS construction through the FP7

EURONS/ISIBHI programme (FY 2005-2008).

• MS-ECRIS has been built in about two years with a contribution of 9 institutions.

• Its design has been based on the GyroSERSE project of INFN-LNS.

• It will upgrade GSI facilities, but it may be useful also for SPIRAL2, LHC,

INFN-LNS (to revive Nuclear Physics,LBNL88”-like) and other

accelerators facility.

• The commissioning was scheduled for the 1st half 2007.

• Non critical delay due to delayed delivery of some mechanical parts.

• Critical delay due to the delivery of magnets and cryostat.

• Gyrotron availability also delayed (not critical because of magnets’ delay).

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 32Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

MS-ECRIS assembly

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 33Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

Hexapole after collar pressing

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 34Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

Cold mass tests

The tests of the cold

mass were successful:

hexapole field reached

78% of the nominal

field after two quenches

and full system

quenched at about

40%.

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 35Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

Additional safety and related delay

The analysis of the cold mass test results took to add additional

safety keys to guarantee the magnetic system safety under non-typical conditions (e.g. injection solenoid energized, the other two not

energized), in which case forces up to 30 tons are generated.

This problem and short circuits one added up a total delay of the project of 8 months.

•Factory tests are scheduled for mid-October

•Final tests at GSI will come one month later.

•All the other components ready to be assembled

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 36Santo Gammino

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Plasma chamberand injection plug

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 37Santo Gammino

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gas inlets

Plasma diagnostics

oven

bias disk cooling

biased disk feedthrough

28 GHz waveguide

14/18 GHz waveguide

water cooling in(28 GHz+ oven + 18 GHz)

Internal flangewater cooling

water cooling out(28 GHz+ oven + 18 GHz)

Injection flange

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 38Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

Injection flange

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 39Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

Figure 1. / a coordinates of the first maximum for the Bessel functions and for the firstderivatives of the Bessel functions.

Positioning of waveguides

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 40Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

Plasma chamber and extraction vacuum chamber

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 41Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

MSMS--ECRISECRIS

28 GHz GyrotronThe 28 GHz-10 kW gyrotron tube used for the testswith SERSE in 2000 have been updated with a new HV power supply and control system.

The tube has beenrecently tested at the CPI factory and the whole generator wastested at 11 kW in France in August. Itwill be moved at GSI this month.

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 42Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

EIS modification

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 43Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

Perspectives

• Assembly of the source will be completed in November.

• First tests will begin in Dec. ‘07 in cw mode, with gas.

• Optimization of beamline, optimum position of biaseddisk and of extraction electrode (+ tests of differentmaterials and dimensions).

• Optimization of cw beams with different magnetic fieldprofile, tests of scaling of Binj, Bext, Brad, Bmin.

• Plasma Diagnostics: X, RF, optical.

• Beam Diagnostics.

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 44Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

•Emittance Measurements.

•Maximum power

•Two Frequency Heating.

•Metal ion beams in cw mode.

•Ion beams from gas and metals in pulsedand afterglow mode.

Perspectives

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 45Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

1. Resistively heated foil oven2. Inductively heated oven

- Above 2000ÚC

- Usability/reliability has to be improved

Metal ion production

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 46Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

2009 and beyond

• Further tests with MS-ECRIS are under consideration

(electron density increase, plasma diagnostics, etc.).

• The ISIBHI partners + ATOMKI + IKF-JWG + IAP are preparing an application for the 7th FP of EU (the Joint

Research Activity COMPLECS)

• If the application will be successful, a completely new experimental and theoretical activity will be pursued with

different sources, including MS-ECRIS as major tool, at leastfor a few months per year.

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 47Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

Q. - What are the perspective experiments

that may guide towards better

understanding of ECR plasma physics and

higher currents/charge states beams ?

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 48Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

•Qualitative explanations of ECR-Heating has been given by the study of the shape of the electromagnetic field generated in the plasma chamber by the injection of microwaves.

•We‘re able to explain many experimental results obtained so far, but qualitative description is not enough, a quantitative evaluation may permit precise prediction for future ECRIS.

•The minimization of the microwave power suggested by our simulations of TFH will improve ECRIS reliability and stability (lower power used for the same beam production decrease the technological criticalities).

I have a dream:less RF power, more beam!

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 49Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

MS-ECRIS’ future

§ Not only operation at f > 35 GHz.

§ Extensive use of diagnostics for the understanding of the processes

that occur in the plasma in order to maximize the amount of ‘useful’

electrons for ionization (warm population) and to minimize the amount

of unwanted’ electrons (hot population).

§Increase of the plasma density (overdense plasma, OXB transition).

§Study and optimization of beam formation in presence of space charge

forces, in connection with beam emittance measurements and beam

transport study.

§Design, construction and coupling with MS-ECRIS of a broadband

generator at a frequency above 35 GHz (GyroTWT?)

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 50Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

0

50

100

150

200

250

300

5 10 15 20 25 30

Xe27

+ [eµA

]

µ-wave frequency [GHz]

ECR

AECR-U

VENUS 18 GHz

VENUS 28 GHz

56 GHz

MS-ECRIS 56 GHz(out of this scale)

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 51Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

Last consideration:

For any kind of ion species,

ECRIS have increased the

current with a rate close to one

order of magnitude per decade

18th Int. Conf. on Cyclotrons & Appl., Oct. 5th, 2007, Giardini Naxos 52Santo Gammino

Istituto Nazionaledi Fisica NucleareLABORATORI NAZIONALI DEL SUD

Last question:

I wonder if we can maintainthis trend for many

decades….

The answer will be given at 28th ICCA !!!