the silicon-tungsten tracker of the dampe mission...for both angle of incidence and impact position....

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The Silicon-Tungsten Tracker of the DAMPE Mission Philipp Azzarello, DPNC, University of Geneva for the DAMPE-STK collaboration 10th International Hiroshima Symposium on the Development and Application of Semiconductor Tracking Detectors

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  • The Silicon-Tungsten Tracker

    of the DAMPE MissionPhilipp Azzarello, DPNC, University of Geneva

    for the DAMPE-STK collaboration

    10th International Hiroshima Symposium on the Development and Application of Semiconductor Tracking Detectors

  • DAMPE (DArk Matter Particle Explorer)

    Philipp Azzarello HSTD10 29.9.2015 2

    Neutron Detector

    Plastic Scintillator Detector

    Silicon-Tungsten Tracker (STK)

    BGO Calorimeter

    Launch: Mid Dec. 2015

    W converter + thick calorimeter (total 32 X0) + precise tracking + charge measurement ➠high energy γ-ray, electron and CR telescope

    Detection of 5 GeV - 10 TeV e/γ, 100 GeV -100 TeV Cosmic Rays

    Complementary to Fermi, AMS-02, CALET, ISS-CREAM

  • The Silicon-Tungsten Tracker (STK)

    • Detection area 76x76 cm2

    • Outer envelope 1.12 m x 1.12 m x 25.2 cm• Total weight: 154.8 kg• Total power consumption: 85 W

    Philipp Azzarello HSTD10 29.9.2015 3

    Main tasks:• Track reconstruction• Photon detection• Charge measurement

  • STK Layout and Structure

    • 12 layers of silicon micro-strip detector mounted on 7 support trays

    • Tray: carbon fiber face sheet with Al honeycomb core

    • Tungsten plates (1mm thick) integrated in trays 2, 3, 4 (from the top)

    • Total ~1 X0 for photon conversion• 8 readout boards on 4 sides (IHEP)• Total 192 modules

    Philipp Azzarello HSTD10 29.9.2015 4

  • STK Silicon Sensors • Single-sided Silicon strip detectors produced by Hamamatsu

    • 9.5 x 9.5 cm2, 768 strips, 121 µm pitch (AGILE geometry) • 320 µm thick (AGILE: 410 µm) • Resistivity 5-8 kΩ, Vfd 10-80 V• Total strip capacitance 2.1 pF/cm

    • 150 SSDs for EQM (Engineering and Qualification Model)• 865 SSDs for FM (Flight Model)

    • Excellent quality• ~120 nA @150V (spec:

  • STK Readout Electronics • Readout every other strip, readout pitch 242 µm• ASIC: VA140 from IDEAS, updated version of VA64hdr of AMS-02

    • Low power (0.3 mW/channel) and large dynamic range (200 fC)• Analog readout

    • Charge measurement• Better position resolution with charge sharing

    • Tracker Front-end Hybrid (TFH) • Thin bias circuit integrated with a PCB housing 6 ASICs, and a readout

    cable (“pigtail”)• Support structure for the SSDs• Vias and copper bands for heat transfer

    Philipp Azzarello HSTD10 29.9.2015 6

  • Silicon Ladder Assembly• Precise jigs to assemble (align, glue and bond) 4 sensors to form a ladder

    Philipp Azzarello HSTD10 29.9.2015 7

  • Silicon Ladders

    Philipp Azzarello HSTD10 29.9.2015 8

    • Alignment precision required: 20 μm • 97% of ladders < 10 μm

    Total leakage current for the 192 installed ladders is excellent

  • Support TraysCFRP plate top

    Al honeycomb

    CFRP frame

    Tungsten plates

    CFRP plate Bottom

    2 CFRP plates of 0.6 mm (or 1 mm for trays with W plates) thick

    4 L-Shape structures in T300 fiber toform the main outside frame.With stainless inserts to connect theTRB frames and the corner feet, andaluminum insert for tray staking

    1 aluminum honeycomb core (37 kg/m3)

    Philipp Azzarello HSTD10 29.9.2015 9

  • Tracker Plane• 16 ladders glued to each surface of the support trays (except top and bottom)

    Philipp Azzarello HSTD10 29.9.2015 10

  • Engineering and Qualification Model (EQM)• An EQM has been constructed in 1st half of 2014

    • full size model as the final Flight Model (FM), but only 26 ladders with real silicon sensors, the rest with dummy sensors

    • EQM passed a series of space environmental qualification tests: vibration, acceleration, shock, thermal cycling, thermal vacuum

    Philipp Azzarello HSTD10 29.9.2015 11

  • Flight Model Assembly• The Flight Model assembly has been completed in April 2015

    • Tested with cosmic rays before delivered to China

    Philipp Azzarello HSTD10 29.9.2015 12

  • Flight Model Status• Since delivery to China:

    • Passed acceptance level vibration and thermal vacuum tests• Integrated into DAMPE final payload, then satellite integration• Passed satellite thermal vacuum tests in orbit simulating vacuum

    chamber• EMI tests

    • STK remain stable through the process• ~0.3% of channels with noise >5 ADC counts (bulk is ~3 ADC counts) • Only 18 (

  • Ladder test beam

    • Two STK ladders have been tested using 400 GeV proton beam at CERN

    • Study the spatial resolution dependence with various angles of incidence.

    • Optimize the charge measurements.• Telescope of Geneva ATLAS group.

    Philipp Azzarello HSTD10 29.9.2015 14

  • Signal identification

    Philipp Azzarello HSTD10 29.9.2015 15

    Cluster identification: • high threshold 4*noise• Low threshold 1.5*noise

    Seed threshold

  • Charge collection

    Philipp Azzarello HSTD10 29.9.2015 16

    Charge distribution for particles hitting perpendicularly the ladder

    For the particles passing close to the floating strip, the collected charge is about 70% of 1-strip clusters.

    Cluster size for different incidence angles

  • Charge collection

    Philipp Azzarello HSTD10 29.9.2015 17

    When the incidence angle increases, the charge is released among more strips and the two peaks shape becomes less evident.

    • The cluster charge for different angles of incidence is compared with a Monte Carlo simulation

    • Charge sharing simulation is based on a spice model• Key parameters: inter-strip capacitance and second neighbor capacitance

  • Philipp Azzarello HSTD10 29.9.2015 18

    • Dependence of the collected charge as a function of the impact point as estimated from the telescope.

    • The strip pitch is of 121 um.• The cluster charge has to be corrected

    for both angle of incidence and impact position.

    Charge collectionangle = 0° angle = 30°

    angle = 60°

  • Spatial resolution

    Philipp Azzarello HSTD10 29.9.2015 19

    • Thanks to the analog readout the spatial resolution is lower than 80 μm for angles below 60°

    • Spatial resolution lower than 50 μm below 40°

  • Summary

    • The Silicon-Tungsten Tracker (STK) of the DAMPE mission is based on robust technology of single-sided silicon strip detectors with analog readout.

    • It will play crucial roles in charge track reconstruction, gamma-ray detection, cosmic ray charge measurement, and overall particle identification.

    • After 2 years of intensive design, prototyping, testing and production efforts• Engineering and Qualification Model was space qualified and tested with

    particle beams• STK Flight Model (FM) completed and passed acceptance and integration

    tests• The quality of the STK is excellent and meets the design specifications

    • Charge collection is studied in terms of impact point and angle of incidence• Within the whole acceptance of STK the spatial resolution is below 80 μm and

    lower than 50 μm below 40°

    • DAMPE will be launched in mid-December 2015

    Philipp Azzarello HSTD10 29.9.2015 20

    The Silicon-Tungsten Tracker �of the DAMPE MissionDAMPE (DArk Matter Particle Explorer)The Silicon-Tungsten Tracker (STK)STK Layout and StructureSTK Silicon Sensors STK Readout Electronics Silicon Ladder AssemblySilicon LaddersSupport TraysTracker PlaneEngineering and Qualification Model (EQM)Flight Model AssemblyFlight Model StatusLadder test beamSignal identificationCharge collectionCharge collectionCharge collectionSpatial resolutionSummary