Shouleh Nikzad Advanced UV/Vis/NIR Detector Arrays and Imaging Systems NASA’s Jet Propulsion Laboratory, California Institute of Technology Pasadena,

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Presentation transcript:

Shouleh Nikzad Advanced UV/Vis/NIR Detector Arrays and Imaging Systems NASA’s Jet Propulsion Laboratory, California Institute of Technology Pasadena, California Presentation Scientific Detector Workshop 2013 Round Table Discussion on Curved Focal Plane Array Florence, Italy 8 October 2013 Curved Focal Plane Array Technologies Enabling Compact, Wide Field of View Optical Systems National Aeronautics and Space Administration © 2013 California Institute of Technology. Government sponsorship acknowledged.

More on Motivation, Solid State CFPAs In a small Panoramic Camera, a CFPA can remove 3-4 elements which improves: Throughput (~order of magnitude) Efficiency Field of view (factor of 2) Image quality (aberration is introduced by each field flattener) Simplicity……… Where were you vacationing last summer?

Curved Arrays have flown on multiple missions Optical layout of FUSE instrument showing curved MCPs on the Rowland circle Curved microchannel plates (MCPs) have been used to enable missions such as FUSE and Alice instrument in Rosetta, however, curved solid state detectors will have clear advantages Also imaging spectrograph Alice has been used on Rosetta, on New Horizon, on LRO (LAMP), and as UVS on JUNO uses MCPs with 75 mm ROC. Called revolutionary because of capability and size.

Challenges: Microchannel plates require high voltage, are bulky, and have low efficiency. Lithography and direct write on curved substrates is expensive and impractical. Require a simple, low-cost method to manufacture CFPAs using solid state detectors. Solution: Decouple VLSI fabrication process from the required curvature Challenges and Solutions Imaging Array

Curved High-purity Silicon Arrays High-purity imagers with full depletion can be back-illuminated without thinning Require a back electrode for depletion Require a back surface treatment to deplete all the way to the surface Imager frontside circuitry High- purity Si Fully-depleted silicon e- photons Delta layer (Thin electrode) Advantages: Simple approach Applicable to fully-processed devices A wide range of shapes and curvatures can be obtained Important factors: Array thickness, array size Silicon purity, depletion voltage, breakdown Near IR variation as a function of thickness

Curved High-purity Silicon Arrays Fabricated PIN diode arrays* to achieve ROC of 260 mm Devices were electrically functional and no punch through was observed. Over depletion is possible Devices responded to light CCDs* with 100 mm ROC was also fabricated. * All LBNL devices =500 nm, RT x Voltage (V)

Curved Silicon Membrane Arrays Advantages: Simple Approach Applicable to front or back illuminated devices Applicable to a wide variety of silicon arrays Compatible with delta doping for high and stable efficiency Challenges: limits of silicon membrane deformation Field effects Thinned membrane arrays conformed or attached to curved substrates Detector Array photons Curved Substrate

Thinned Curved CCD Arrays 1K x1K, 12 µm pixel CCDs were thinned and attached to curved substrates ROC=250 mm For comparison, same CCD formats were thinned and attached to flat substrates Curved Flat Curved Flat

Results of Thinned CFPA, continued Air pressure: 14 psi, ROC ~ 500 mm Light Intensity (arb units) Preamp Output (mV) Air Off (flat) Air On Air pressure, 22 psi, ROC~250 mm Light Intensity (arb units) Preamp Output (mV) Air Off (flat) Air On Freestanding thinned membrane CCDs were curved to different curvatures using air pressure CCD was operated and output current was measured as a function light intensity for CFPAs with three different radius of curvature (ROC) No change in the signal level or device behavior was observed as a function of curvature

Experimental Results of Thinned CFPA Freestanding thinned membrane 1k x1k pixel CCDs were curved to different curvatures using air pressure CCD was taken from essentially flat configuration to ~250 mm radius of curvature (ROC) with no observed mechanical damage

Imaging Results of Thinned CFPA Freestanding (Before Image) Positive 0.1 psi Positive 0.2 psi Negative 0.2 psi Freestanding (After Image) Negative 0.1 psi

Example: Explorer-ISTOS Concept A GALEX follow on mission, benefits from curved detector arrays Preliminary work demonstrated a CCD array, thinned to 20 microns membrane and curved (supported) with ROC ~ 12 mm, far beyond ISTOS requirements. Strain for this severe curvature is 0.1% (limit of Si is 1%)

Curved Wide Bandgap Arrays - Bandgap Selective - Dopant Selective ECEC EVEV EFEF GaNElectrolyte n-GaN p-GaN Pt Cathode Aqueous KOH (pH ~14) UV (Xenon Arc Lamp) p-AlInGaN ProtectedMUX n-GaN Opaque Mask Holes created by UV light are swept away from surface in p-type, towards surface in n-type -> n-type etching Photo-ElectroChemical Etching (PEC) of GaN

What does NASA space technology have to do with neuroscience, neurosurgery, or medicine? NASA Requirements: Great efforts and resources go into developing technologies and instruments to detect signatures from faint objects, characterize planetary atmospheres, detect remnants of dying stars, explore planetary bodies, look for signs of life… These require high sensitivity, high accuracy, reliable, robust, compact, low power, low mass, non-invasive instruments that can work in harsh and unfriendly environments

Should Sound familiar to Medical Doctors Requirements in medicine We as a people are/should be willing to spend great efforts and resources to help patients. We try to detect faint signals to delineate good cells from bad, get close to the area of interest without disturbing others, look for signs of life… These conditions require high sensitivity, high accuracy, reliable, robust, compact, low power, low mass, non-invasive instruments that can work in unfriendly environments There is great synergy and a great deal to leverage from. With relatively small investment great gains can be achieved!

Summary Curved focal plane arrays enable large FOV, high throughput, low mass, and compact optical systems The key to a practical (and low cost) fabrication approach for CFPAs is to decouple the VLSI fabrication from the required curvature We have demonstrated multiple simple, practical approaches for fabrication of CFPAs Simple modeling was performed to investigate deformation thinned membrane arrays Some of the techniques were extended to GaN materials and devices

Backup Slides

Two-element simplification of design (elimination of field flatteners) Some Motivations for CFPAs Optical wave fronts are curved and don ’ t match the FPAs Field flatteners are used to match the FPA Allowing the FPA to be curved will: >eliminate optical elements > Reduce size and mass > Reduce complexity > Increase throughput and image quality > Dramatically increase the field of view (FOV) >Allow designer more parameters Wide FOV, severely curved, needs only 2 optical elements Wide FOV, essentially flat, needs 11 optical elements Table qualitatively shows that optical systems with the same focal length (FL), field of view (FOV), allowing the FPA to be curved, reduces the number of optical elements

Evolution of CCD flatness Experimental Methods for CFPAs using Thinned Membranes Vacuum conforming of imagers (full contact) Pressure conforming of Imager Thinned membranes can be conformed to substrates for flat or curved focal planes Real time adjustment of curvature possible with no substrate attachment Detector Array Curved Substrate

Large Focal Plane Arrays Frontside circuitry photons Mosaics of curved detector arrays can form a large focal plane array that can be curved to the specifications of the system flat

Imaging Results of Thinned CFPA

Conforming Thinned Silicon Smaller arrays accommodate tighter ROCs, larger arrays require gentler ROCs, Mosaiced arrays can accommodate a larger range of ROCs Silicon has a mechanical deformation limit of 1.0 percent Conforming a square array onto spherical substrate Sharpest Radius of Curvature for 0.01 Strain Square Array Side (mm) Radius of Curvature (mm)

Elastic Deformation - Basic Equations Displacement field: Static equilibrium equation: Stress and strain fields: Finite Difference Analysis for Membrane Deformation

Si Membrane - Model R H Cylindrical symmetry Boundary conditions: 0 1) Contact with sphere: 2) Hydrostatic pressure: Pressure on element with norm n i : on sphere on free surface “ clamped edge ” on pressurized surface on free surface “ clamped edge ” Finite Difference Analysis for Membrane Deformation

Numerical Implementation Uniform Cartesian grid in (r,z) plane: N r points along the radius N z points along the thickness r z Finite difference discretization: Finite Difference Analysis for Membrane Deformation

Results of Analysis for Hydrostatic Pressure Membrane radius = 2 mm Membrane thickness H = 5  m Pressure = 5 * Young modulus Radial strain Radial displacement Vertical displacement P

Analysis Results for Full Contact With Sphere Membrane: radius = 2 mm thickness H = 5  m Sphere in full contact: Strain Displacement