Advanced OST System for the Second-sound Test of Fully ... · 20.07.2017 Y.Tamashevich, SRF2017...

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ADVANCED OST SYSTEM FOR THE SECOND-SOUND TEST OF FULLY DRESSED CAVITIES Y. Tamashevich Helmholtz-Zentrum Berlin for Materials and Energy (HZB), Berlin, Germany also at University of Hamburg/DESY, Hamburg, Germany [email protected]

Transcript of Advanced OST System for the Second-sound Test of Fully ... · 20.07.2017 Y.Tamashevich, SRF2017...

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ADVANCED OST SYSTEM FOR THE SECOND-SOUND TESTOF FULLY DRESSED CAVITIES

Y. TamashevichHelmholtz-Zentrum Berlin for Materials and Energy (HZB), Berlin, Germany

also at University of Hamburg/DESY, Hamburg, Germany

[email protected]

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ρ= ρn+ ρs

Superfluid Helium and Second Sound

Helium phase diagram Phase fractions

- first sound

- second sound

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Quench in the cavity deposits heat into the helium bath

Second sound wave is induced

Temperature or phase oscillations can be detected

Quench

He He

He He

Previous talk byH. Furci

This talk

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Cathode: porous “superleak” membrane

Bronze anode

Dielectric epoxy

Aluminum housingAluminum cap

SMA connector

6 um thick polycarbonate125 nm pores (3% of the surface area)45 nm gold layer on one side

1 cm

Only superfluid can flow through (at a given ω)

Full density ρ= ρn+ ρs oscillates behind the membrane

Membrane moves*

Capacitance of the OST changes

Oscillating Superleak Transducer (OST)

Cornell design: Z.A. Conway, D.L. Hartill, H.S. Padamsee, E.N. Smith,“Oscillating Superleak Transducers For Quench Detection in Superconducting ILC Cavities Cooled with He-II”,TESLA Technology Collaboration, Ithaca, New York, 2008.

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Signal acquisitionAmplification circuit

Noise level

SNR spectrum of OST signal

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Signal amplifier

Noise levelSNR spectrum of OST signal

-18V

+96V Low dropoutregulators (LDO)

Single-channel

+90V to OST

Signal to ADCPower supply 8-channel amplifier+18V

Low-noise, wall-plug powered

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Up to 18 signals are acquired simultaneously

OST Detection time

Quench distance=

OST Signals

OST detection time

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OST Signals

The simplest way to locate the quench is trilateration.

• Low accuracy (quench in few cm from the surface )• Uses only OSTs “in sight”• Do not use the signals of “hidden” OSTs(i.e. 4-5 signals of 18 are used)• Requires many OSTs to cover the full surface

Trilateration – not precise

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The shortest path from any point on the cavity surface to the OST can be calculated using the cavity shape

Ray tracing

Path of the wave around the cavity (simple mesh)

Possible paths of the wave (2D)

OST

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3D simulations are used to find the shortest paths of second sound from the quench point to each OST.

Results of 3D simulations and path calculations are stored in 2D matrices which allows using of these precalculated results during the second sound tests.

Dumbbell shape with normal vectors and triangular mesh

Graph of Interconnections

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r35 r34 r33 r32 r31 r30 r29

r28 r27 r26 r25 r24 r23 r22

r21 r20 r19 r18 r17 r16 r15

r14 r13 r12 r11 r10 r9 r8

r7 r6 r5 r4 r3 r2 r1

0°180° angle

heig

ht

0

HDistance matrix

anglez a

long

surf

ace

Distance map

Assumptions:• The quench origin is located on the cavity surface

• The second-sound wave reaches the OST by taking the shortest possible route

• The velocity of second sound in helium is constant for the whole volume of the cryostat

developed view of the cavity surface

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For each point of the map all OST signals are linearly fitted by the second sound velocity (19.9 m/s at 1.8 K)4

Calc

ulat

ed d

istan

ce

measured time

Heat propagation effect

4Russell J. Donnelly - The Observed Properties of Liquid Helium at the Saturated Vapor Pressure

Combination of n Distance maps

Quench Localisation

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OSTs in direct view OSTs without direct view

The OSTs both in direct view and without direct view can be used to determine the quench position

Can be also done by trilateration Can be done only by path calculation

Detectors in direct view and without direct view of the quench point

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Second Sound map T-map

T-mapping shows the quench point close to the spot defined by the Second Sound test

Comparing with T-mapping results (naked cavity)

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Dressed Cavities

bERLinPro booster cavity4 OST are installed in a helium pipe

4 9-mm OSTs assembledon a plastic holderOST size is strongly limited to allow

sufficient cavity cooling

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6 sensors

Dressed Cavities - Multi-OST

Multi-OST Multi-OST installed into the helium pipe

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Multi-OST: various dimensions

38 mm, 8-channel multi-OST 52 mm, 6-channel multi-OSTin a helium tank of the cavity

Multi-OST of various dimensions and with different number of channels were developed.

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Ready-to-use system for E-XFEL cavities

• Designed to be repeatedly used • Provides precise positioning of the sensor• Does not require any additional cavity preparations

Need less than 2 minutes for mounting

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A part of the quench map for the dressed cavity

Results: Standard E-XFEL cavity with tank

CAV00683

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Optical image (OBACHT) Laser image of the replica

Welding seam of the Equator 9 at 50 °

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Laser image 3D image

Profile of the defect

Profile of the defect

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Algorithm

MatLab code is available on GitHub

The most intensive calculations Cold Test

• The most intensive calculations (building the graph) are separated and done once for the cavity shape used.

• Distance maps should be calculated for the specific OST positions. If the same OST positions are used, the same distance maps can be used.

• Calculation of the quench map can be done “on-the-fly” during the cavity test

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• The hardware and algorithm for second-sound tests were developed and verified by testing 9-cell cavities.

• The precision of localisation of the quench is in a good agreement with the direct temperature measurements.

• A multi-OST for the second-sound test of a series-production XFEL cavity was developed.

• Such a system can be used with different cavity shapes and sizes.

Second Sound: Results

A second sound test is proposed to be a part of a standard vertical test.

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We acknowledge help of DESY collegues:

J. Eschke,A. MattheisenD. ReschkeT. KuelperA. Navitski.

Acknowledgements

Special thanks to:

E. Elsen, CERNB. Foster, University of Hamburg

A. Neumann, HZBJ. Knobloch, HZB

Thank you!

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