spectroscopy of breakdowns breakdown physics workshop j.kovermann 6.5.2010

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Spectroscopy of breakdowns Breakdown physics workshop J.Kovermann 6.5.2010

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Page 1: Spectroscopy of breakdowns Breakdown physics workshop J.Kovermann 6.5.2010

Spectroscopy of breakdowns

Breakdown physics workshopJ.Kovermann

6.5.2010

Page 2: Spectroscopy of breakdowns Breakdown physics workshop J.Kovermann 6.5.2010

How it fits into the CLIC study:

ComprehensiveRF design

RFmeasurements

DCmeasurements

High-power scaling

laws

Breakdown simulation

Breakdown diagnostics

New experimental techniques complementary to RF tests

Page 3: Spectroscopy of breakdowns Breakdown physics workshop J.Kovermann 6.5.2010

Breakdown diagnostics

BREAKDOWNDIAGNOSTICS

Spectroscopy,Integrated and time-

resolved

Plasma parameters

simulation input

Plasma composition simulation and mat.sci.

input

OTR in nominal pulses simulation and machine

parameter input

RF measurements, FC, XRAY simulation and design input

SEM simulation and design

input

Missing energy ?

Plasma size/position simulation and design

input

Page 4: Spectroscopy of breakdowns Breakdown physics workshop J.Kovermann 6.5.2010

Spectroscopy in rf and dcSubject of my thesis:

Comparative studies of rf and dc breakdowns by optical spectroscopy

Task: Show validity of dc breakdown experiments for rf simulation and design

Approach: Time integrated and time-resolved spectroscopy of dc and rf breakdowns

Dc experiments are faster and easier, e.g. few CHF per sample, up to kHz rep.-rate with new power supply (end 2010) Two dc setups available at CERN, others under construction Less scheduling issues

Page 5: Spectroscopy of breakdowns Breakdown physics workshop J.Kovermann 6.5.2010

Time-integrated spectroscopySpectrograph and CCD camera

Dc breakdown, 400MV/m, 0.93J

Int. ratio lines/continuum = 1/4

Page 6: Spectroscopy of breakdowns Breakdown physics workshop J.Kovermann 6.5.2010

Time-integrated spectroscopySpectrograph and CCD camera

Rf breakdown, 40MW, 200ns, 8J, SLAC C10

Fast failure diagnostics!

Page 7: Spectroscopy of breakdowns Breakdown physics workshop J.Kovermann 6.5.2010

Time-integrated spectroscopyReproducibility and comparison

Rf, 37MW, 200ns, C10, 17 BDs DC, 8kV, 0.98J, Cu, 499 BDs

Remarkably reproducible after normalization to total intensity !

Page 8: Spectroscopy of breakdowns Breakdown physics workshop J.Kovermann 6.5.2010

Time-integrated spectroscopyReproducibility of line-ratios

Line ratios are constant over many breakdowns in rf and dc TLM applicable? (dc: 4280K±9K, rf: 5366K±61K) TLM not consistent for all line pairs!

Page 9: Spectroscopy of breakdowns Breakdown physics workshop J.Kovermann 6.5.2010

Time-integrated spectroscopyLine-ratios and total intensity

Line intensity / total intensity is spreading towards shorter wavelengths Line ratios are only weakly connected to dissipated energy

Page 10: Spectroscopy of breakdowns Breakdown physics workshop J.Kovermann 6.5.2010

Time-integrated spectroscopyNo breakdown OTR

Dc, 4.25kV, Cu, 600s int.

Rf 30GHz SBS, 66MV/m 1h int.

Light present when electric field is applied

Shoulder at 2.1eV (interband transition)

OTR light present in dc and 30GHz rf, not found in X-band rf…

Page 11: Spectroscopy of breakdowns Breakdown physics workshop J.Kovermann 6.5.2010

Time-integrated spectroscopyNo breakdown OTR

The Mo OTR mystery:

Why only these two lines?

694.7nm MoI

693.4nm MoI

Page 12: Spectroscopy of breakdowns Breakdown physics workshop J.Kovermann 6.5.2010

Time-integrated spectroscopyNo breakdown OTR field enhancement factor

New way of measuring β close to the breakdown threshold (impossible with current dc setup)

Page 13: Spectroscopy of breakdowns Breakdown physics workshop J.Kovermann 6.5.2010

Time-resolved spectroscopyPower and light waveforms

Dc: Max. light emission after max. power Rf: Light lasts longer than input power

Dc

Rf

Page 14: Spectroscopy of breakdowns Breakdown physics workshop J.Kovermann 6.5.2010

Time-resolved spectroscopyConsistency with integrated spectroscopy

Time-resolved (PMT) and integrated (CCD) spectroscopyshow consistent results, even though the method and number of BDs are totally different

Acquired time-resolved with PMT, integrated

by computer afterwards (20BDs averaged per bin)

Integrated by CCD camera (single BD)

Page 15: Spectroscopy of breakdowns Breakdown physics workshop J.Kovermann 6.5.2010

Time-resolved spectroscopyContinuum and lines

Dc: Spectrum consists of continuum and lines

continuumlines

Page 16: Spectroscopy of breakdowns Breakdown physics workshop J.Kovermann 6.5.2010

Time-resolved spectroscopyReproducibility of emission waveforms

Dc: Waveform reproducible, lines emit longer than continuum

522nm 516nm

518nm(background)

Page 17: Spectroscopy of breakdowns Breakdown physics workshop J.Kovermann 6.5.2010

Breakdown spectroscopyConclusion

Spectra of rf and dc breakdowns show Cu ions up two CuIII Other elements were not identified (but still one unidentified broad line) Main emission intensity originates from continuum Continuum emission ends before line emission and is weaker Total intensity of spectrum scales with line intensity and vice versa Non-LTE plasma, temperature calculations are inconsistent

OTR emission seen in rf and dc Cu OTR spectrum modulated by Cu reflectivity OTR light is linear proportional to current (and rel. factor) Can be used to get field enhancement factor close to breakdown limit

High electric noise environment, very low light levels, fast processes and (yet) unpredictable position (rf structures!!) complicates experiments a lot!

THANK YOU!