Photon Counting Sensors for Future Missions Dr. Oswald Siegmund Space Sciences Laboratory University of California, Berkeley, CA FUSE rowland circle 200 x 10mm curved MCP detector, 10k x 300 form GALEX 65mm MCP sealed detecto rs, 2k x 2k format 130nm - 300nm M31/32 Imaging Spectroscopy
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Photon Counting Sensors for Future Missions Dr. Oswald Siegmund Space Sciences Laboratory University of California, Berkeley, CA FUSE rowland circle 200.
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Photon Counting Sensors for Future MissionsDr. Oswald Siegmund
Space Sciences LaboratoryUniversity of California, Berkeley, CA
FUSE rowland circle 200 x 10mmcurved MCP detector, 10k x 300 formatGALEX
65mm MCP sealed
detectors,2k x 2k format
130nm -300nm
M31/32
Imaging
Spectroscopy
QuickTime™ and aGraphics decompressor
are needed to see this picture.Experimental Astrophysics Group
Historical Progress of Spatial Resolutionfor photon counting sensors
Imaging and spectroscopy MCP sensors for past and future missions. All sciencetopics show rapid rise in spatial resolution performance requirements.Astronomy/solar sensors are most demanding. Remote sensing less so but have greater timing needs. Planetary sensors emphasize low power/weight
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AstronomyRemote SensingPlanetarySolar
Date
HORUS
MUST
NPOESS
COS
STIS
FUSE
JMEX
NEXUS
EUVE
JUNO
GALEX
IMAGE SI
IMAGE EUVI
PLUTOALICE
ROSETTA ALICE
IMAGER
GUVI
IMAGE WIC
ALEXIS
ORFEUS
SOHO
FAUST
Photon Counting Sensor CharacteristicsNo cosmic ray streaks
No need for accurate pointing stability during long exposures
Cosmic rays rejected, or just dots.
No radiation damage.
Photons time tagged, rebin image with aspect solution
No degradation of cathode QE with time or environment
No cooling required. No need for de-contamination. No CTE changes
No transfer of blank data areas, no noise pedestal
Only photon events and photon-like background registered
Register position and time with electronic readout
Schematic for cross strip readout
High Quantum Efficiency PhotocathodesNew III-V photo-cathodes are under development
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GaN JG-138
NW-BH071#3
GaN JG-138
SVT3102#2
GaN JG-220
Wavelength (nm)
Early trial sealed tube
Process development samples
& significant improvements in QE are being made
GaAs photocathodes overlapGaN and have high QE into IR
GaN opaque photocathodesshow high QE and longevity
QE @ 600nm < 10-6
STIS
Other materials also show promise, diamond, othe III-V compounds
Advanced Microchannel Plates
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Background Rate (events cm
-2
sec
-2
)
Threshold (x modal gain)
Residual counts from glass MCP's?
Photo-lithographic silicon based MCP’s - uniform pore pattern. No multifiber boundaries & array distortions of glass MCP’s. Large substrate sizes (100mm) OK, with small pores (<5µm). High temperature tolerance - CVD cathode processes OK. Initial tests are encouraging, but needs more development
Si MCP ~7um hex pores, >75% OAR
Ultra low background rates<0.02 events cm-2 sec-1
8cm Si MCP on 100mm wafer
Diamond on Si MCP
Cross Strip Imaging Readout
Air force mask on 7µm pore MCP pair with 32mm cross strip
Cross strip is a multi-layer cross finger layout.
Event charge centroid gives event positions.
Ultra high spatial resolution (<5µm)
Large formats possible (100mm) in many shapes
Low gain/long lifetime/low fixed pattern noise
Anodes 32 x 32mm have been made.
7µm pore MCP pair at 2x106 gain
ASIC preamps plug directly to
the anode
Gain 4 x 105
MEDIPIX (CMOS) readout for MCP’s
Cathode + MCP + image readout using “Medipix2” ASIC by CERN.