Air Force Research Laboratory Lead ~ Discover ~ Develop ~ Deliver Multimodal Data and Anomaly Detection in SSA at AMOS 15 Oct 2012 Dr. Keith Knox Air Force Maui Optical & Supercomputing Site Maui, Hawaii Photo of Briefer Air Force Maui Optical & Super Computing Site 2 Air Force Maui Optical & Supercomputing Site 50 Years of Service to the Department of Defense 1960: The Advanced Research Projects Agency (ARPA) Midcourse Optical Station 1963: Site construction started by ARPA 1994: High Performance Computer Center (HPCC) completed 1999: Advanced Electro-Optical System (AEOS) completed 2001: Air Force Research Laboratory • Largest telescope in Department of Defense with 3.6m primary telescope • Highest resolution adaptive optics in Department of Defense • Largest electro-optical tracking facility in the Pacific 3 Air Force Research Laboratory Directed Energy Directorate Maui Space Surveillance System MSSS (AFRL) 3.6m and 1.6m telescopes Maui Space Surveillance System 1.6m • • • High-resolution Imaging Orbital Tracking Space Object Characterization AEOS 3.6m GEODSS (AF Space Command) Ground-based Electro-Optical Deep Space Surveillance GEODSS 4 3.6-meter Telescope AEOS 3.6 Telescope Advanced Electro-Optical System 5 1.6-meter Telescope 1.6 Meter Telescope Inside Dome 6 Adaptive Optics Imaging AEOS Visible Imager Day Terminator Night Hubble Space Telescope Adaptive Optics (AO) plus multi-frame blind deconvolution processing • Terminator Imagery 7 Long-Wave Infrared Imaging AEOS Infrared Imager Day Terminator Night • Resolved thermal images • Virtually diffraction-limited • Nighttime Imagery 8 Speckle Imaging Speckle Imaging 1.6m Day Terminator Raw data Processed Result Night • Daytime Imagery • Terminator Imagery 9 Non-imaging Characterization • As satellite image size decreases … – Smaller satellite – Greater distance • the satellite becomes completely unresolved – Satellites in geo orbit – Cubesat-class satellites 10 Non-Imaging Technique • Temporal filter photometry – Measured brightness as function of time • For an object facet to contribute to signal – Facet must be illuminated by Sun – Facet must be visible to sensor Temporal photometry • Sensor requirements are simple – Calibrated light bucket 11 Astrodynamics & Tracking High Performance Computing Software Applications Institute for Space Situational Awareness Now 15k Objects Good orbit knowledge and some status info Future 150k Objects Accurate orbits and uncertainty Object identification status and health The Institute meets these challenges by bringing together: • Supercomputing expertise • World-class researchers from AFRL 12 Anomaly Detection and Multimodal Data in Astrodynamics 13 Space Catalog Anomalies • 22,000 objects in the catalog • What is an anomaly? – – – – – New satellite is launched Debris is created Satellite maneuvers Object drifts Satellite status has changed • Track 22K objects – Look for deviations • Paul Schumacher – “The Future Space Catalog” 14 Multimodal Space Catalog: Radar vs. Optical 2 radar observations Range1 Az1 Elev1 3 optical observations Range2 Az2 Elev2 RA1 Dec1 RA2 Dec2 RA3 Dec3 2 observations 6 scalars ( x y z vx vy vz ) 6 scalars 3 observations 6 scalars ( x y z vx vy vz ) 6 scalars Radar and Optical Observations translated into 3-D spatial coordinates 15 Observation Association is Hard ? ? SST ? ? Space Surveillance Telescope For one object, all observations are connected For many objects, all observations are connected 16 Multimodal Data in Speckle Imaging 17 Speckle Imaging using Short Exposure Sequences • High resolution details are lost in long exposures through the atmosphere: • However, detail is encoded in short exposure images: • Assume that target is constant over period of a few seconds. Then image reconstruction is possible: 18 Speckle Imaging Multi-Frame Blind Deconvolution (MFBD) Noisy and blurred images Blurring functions True object h1x i1x ox h1x n1x o(x) h2 x i2 x ox h2 x n2 x … … hN imagesx Restored object iN imagesx ox h N imagesx nN imagesx MFBD Processing Minimize this cost function with respect to oˆ x , hˆ 1 x , … , hˆ N x : images oˆ x Nim agesNpix els k 1 n 1 i x ˆi x σ x 1 k 2 k n n k 2 n 19 Multimodal Data Improves Image Reconstruction • Each wavelength experiences ~same optical path difference (OPD) due to atmospheric turbulence • Wavefront phase is θλ = OPD × 2π/λ OPD in telescope pupil Infrared images define OPD, which in turn improves visible reconstruction Brandoch Calef, “Wavelength Diversity” 20 Multimodal Data in Non-Imaging 21 Spectrophotometry with BASS at AEOS •IR spectrophotometry in 3-13.5 mm range •Princeton CCD camera & filter collect images simultaneously with IR spectra 22 22 Modeling Reflected & Emitted Radiation • Modeling space debris to match simultaneous IR and visible response • HAMR objects – High Area-to-Mass Ratio • Mark Skinner – “Fusing Visible and Thermal IR Signature Data for SSA” 23 Anomaly Detection in Non-Imaging 24