A novel hyperspectral imager based on microslice technology A novel hyperspectral imager based on microslice technology Ray Sharples, Danny Donoghue, Robert.

Slides:



Advertisements
Similar presentations
Remote sensing, promising tool of the future Mária Szomolányi Ritvayné – Gabriella Frombach VITUKI CONSULT MOKKA Conference, June
Advertisements

HIRES Technical concept and design E. Oliva, HIRES meeting, Brera (Milan, Italy)1.
1 ATST Imager and Slit Viewer Optics Ming Liang. 2 Optical layout of the telescope, relay optics, beam reducer and imager. Optical Layouts.
CHRIS (Compact High Resolution Imaging Spectrometer) sira group sira electro-optics Dr Mike Cutter EO & Technology Business Manager.
Some Basic Concepts of Remote Sensing
Resolution.
Doppler Wind and Temperature Sounder: A breakthrough technique GATS Proprietary Larry Gordley, GATS Inc. Dave Fritts, GATS Inc. Tom Marshall, GATS Inc.
Line scanners Chapter 6. Frame capture systems collect an image of a scene of one instant in time The scanner records a narrow swath perpendicular to.
Remote sensing in meteorology
Preliminary Performance Measurements for Streak Camera with Large-Format Direct-Coupled CCD Readout* 15th Topical Conference on High-Temperature Plasma.
1 PHYSICS Progress on characterization of a dualband IR imaging spectrometer Brian Beecken, Cory Lindh, and Randall Johnson Physics Department, Bethel.
Hyperspectral Imagery
Wide-field, triple spectrograph with R=5000 for a fast 22 m telescope Roger Angel, Steward Observatory 1 st draft, December 4, 2002 Summary This wide-field,
SWIFT Team University of Oxford 12 th November 2007O-SWIFT Progress Report Fraser Clarke.
Astronomical Spectroscopy
KMOS Instrument Science Team Review Instrument overview.
2010 CEOS Field Reflectance Intercomparisons Lessons Learned K. Thome 1, N. Fox 2 1 NASA/GSFC, 2 National Physical Laboratory.
Astronomical Instrumentation Often, astronomers use additional optics between the telescope optics and their detectors. This is called the instrumentation.
T-REX OU4 HIRES The high resolution spectrograph for E-ELT E. Oliva, T-REX meeting, Sexten Pustertal (I)1.
Satellite Imagery and Remote Sensing NC Climate Fellows June 2012 DeeDee Whitaker SW Guilford High Earth/Environmental Science & Chemistry.
1 Remote Sensing and Image Processing: 7 Dr. Mathias (Mat) Disney UCL Geography Office: 301, 3rd Floor, Chandler House Tel: (x24290)
Blue: Histogram of normalised deviation from “true” value; Red: Gaussian fit to histogram Presented at ESA Hyperspectral Workshop 2010, March 16-19, Frascati,
Resolution A sensor's various resolutions are very important characteristics. These resolution categories include: spatial spectral temporal radiometric.
Christine Urbanowicz Prepared for NC Climate Fellows Workshop June 21, 2011.
14 October Observational Astronomy SPECTROSCOPY and spectrometers Kitchin, pp
18 October Observational Astronomy SPECTROSCOPY and spectrometers Kitchin, pp
Remote Sensing and Image Processing: 7 Dr. Hassan J. Eghbali.
DL – IFU (Prieto/Taylor) Slicer: –25mas sampling … 0.9mm slices ~f/250 (assuming no anamorphism) Detector = 2k array of 18um pixels –Slit subtends 1-pixel.
1 Applications of Remote Sensing: SeaWiFS and MODIS Ocean Color Outline  Physical principles behind the remote sensing of ocean color parameters  Satellite.
Integral Field Spectroscopy. David Lee, Anglo-Australian Observatory.
An IFU for IFOSC on IUCAA 2m Telescope
TIDAS-SPU: Development and testing of a system for infrared FTS imaging of the atmosphere Neil Humpage 1, John Remedios 1, Alex Wishart 2, Thomas McCoy.
The Study of IFU for the Li Jiang 2.4m Telescope ZHANG Jujia 张居甲 Yun Nan Astronomical Observatory. CAS Sino-French IFU Workshop Nov Li Jiang.
KMOS Instrument Overview & Data Processing Richard Davies Max Planck Institute for Extraterrestrial Physics  What does KMOS do?  When will it do it?
WFIRST IFU -- Preliminary “existence proof” Qian Gong & Dave Content GSFC optics branch, Code 551.
イメージスライサー型可視光 面分光ユニットの開発 Development of an integral field unit (IFU) with an image slicer Shinobu Ozaki, Satoshi Miyazaki, Takuya Yamashita, Takashi Hattori,
Mirza Muhammad Waqar HYPERSPECTRAL REMOTE SENSING - SENSORS 1 Contact:
1 Access and Use of Auroral Imaging Data Harald U. Frey Space Sciences Laboratory University of California at Berkeley Credit: D. Hutchinson.
Hyperspectral remote sensing
OMI validation workshop - 22 nd June 2006 Louisa. J. Kramer (1), Paul. S. Monks (2), Roland. J. Leigh (1) (1) Earth Observation Science, Space Research.
Use of Solar Reflectance Hyperspectral Data for Cloud Base Retrieval Andrew Heidinger, NOAA/NESDIS/ORA Washington D.C, USA Outline " Physical basis for.
NIRSpec IFU Eric Prieto Final Presentation Definition Phase May, 11th – ESTEC.
Science with Giant Telescopes - Jun 15-18, Instrument Concepts InstrumentFunction range (microns) ResolutionFOV GMACSOptical Multi-Object Spectrometer.
Astronomical Observational Techniques and Instrumentation
Visible Spectro-polarimeter (ViSP) Conceptual Design David Elmore HAO/NCAR
Sub pixelclassification
Demonstration of Low Spatial Frequency Restoration for a Phased Sparse Aperture Telescope Array Tomás Avilez Industrial Affiliates.
Sample expanded template for one theme: Physics of Galaxy Evolution Mark Dickinson.
F. Pepe Observatoire de Genève Optical astronomical spectroscopy at the VLT (Part 2)
Electro-optical systems Sensor Resolution
UNIT 2 – MODULE 5: Multispectral, Thermal & Hyperspectral Sensing
2015 GSICS Annual Meeting, Deli India March 16~20, 2015 Xiuqing Hu National Satellite Meteorological Center, CMA Yupeng Wang, Wei Fang Changchun Institute.
Integral Field Spectrograph Eric Prieto LAM. How to do 3D spectroscopy.
Single Object Spectroscopy and Time Series Observations with NIRSpec
Hyperspectral Sensing – Imaging Spectroscopy
Single Object & Time Series Spectroscopy with JWST NIRCam
GEOGRAPHIC INFORMATION SYSTEMS & RS INTERVIEW QUESTIONS ANSWERS
JWST NIRCam Time Series Observations
Hyperspectral Remote Sensing
VIRTIS Operations at Lutetia
ESAC 2017 JWST Workshop JWST User Documentation Hands on experience
An IFU slicer spectrometer for SNAP
Changchun Institute of Optics Fine Mechanics and Physics
Early calibration results of FY-4A/GIIRS during in-orbit testing
Preliminary SCIAMACHY Lunar observations as intercalibration source
How we do Spectroscopy An Overview
Remote sensing in meteorology
Hyperspectral Remote Sensing
X-ray high resolution spectra in the VO: the case of XMM-Newton RGS
Presentation transcript:

A novel hyperspectral imager based on microslice technology A novel hyperspectral imager based on microslice technology Ray Sharples, Danny Donoghue, Robert Content Colin Dunlop, David Nandi, Gordon Talbot Durham University UAV Workshop 7 th July 2011

Outline of Presentation Background Background Methods for simultaneous 3D spectroscopy Methods for simultaneous 3D spectroscopy Operating principles of a microslice hyperspectral imager Operating principles of a microslice hyperspectral imager First laboratory results from a CEOI- funded prototype sensor First laboratory results from a CEOI- funded prototype sensor Future Plans Future Plans

Project Background TelescopefocusSpectrographinput Lensletarray Fibrearray Imageslicer 1234 Both designs maximise the spectrum length and allows more efficient utilisation of detector surface. Only the image slicer retains spatial information within each slice/sample  high information density in datacube Overlaps must be avoided  less information density in datacube Spectrographoutput slit Fibres Pupil imagery slit Micro- mirrors x y Datacube Divides the field in two dimensions

Project Background

Fully exploit modern large-format 2D detectors to obtain faster survey speeds. Longer exposures in stare-mode to allow higher SNR in finer pixels for radiometry, meteorology & and atmospheric composition studies - particularly important for low reflectivity targets such as water, forestry and shallow marine environments. Enable smaller, more compact devices than other comparable platforms. Compact designs using state-of-the-art sensors to reduce mass/volume requirements. Step-change in the imagery available to assist in meeting NERC targets for Earth observation with applications in many areas: not in the least vegetation, geology and pollution monitoring. CEOI Seedcorn Project: budget £50k. A New Approach to Hyperspectral Imaging V km/sec xx Dwell time =  x/V

Instrument Concept: Microslice IFU

Instrument Layout CEOI Mid-Term Review Meeting 12 Jan 2011 Pick-off mirror Collimator Image slicer Fore-optics GRISM Camera Baseplate (cover omitted) Dimensions 33 cm x 15 cm x 12 cm Mass ~5 kg (excl baseplate)

Hyperspectral Imaging Using Microslice Technologies Novel application of microlens resampling optics to deliver unprecedented field-of-view sampling over multiple spectral channels simultaneously. Addresses current spectral resolution and sensitivity limitations with available airborne/spaceborne instruments. Enables high spectral resolution observations to characterise and quantify ecosystem and land/water surface properties. Allows spectral fingerprinting to be scaled up to address whole Earth system processes.

Prototype Microslice Spectrograph NERC Centre for Earth Observation Instrumentation Seedcorn Project started April x 20 “spaxels” (spatial pixels each giving a spectrum) so 6,600 spectra. Spectra 180 pixels long Resolution of 5-7 nm (slice images 3 pixel wide) over 400 nm to 700nm Dimensions 33 cm x 15 cm x 12 cm

Microslicer Assembly

Microslice Optical Performance

Foveon CCD

Flatfield Performance nm

Spectral Performance H beta H alpha Hg

Application Tests Lab set up Microslicer & ASD FieldSpec Pro Objectives: – Test spectral resolution – Test signal / noise ratio – Ability to extract spectra – Use Spectralon standard

Calibration and Testing

565 nm Fagus sylvatica leaf Calibration and Testing Source: David Nandi

Extracting spectra from datacube Source: David Nandi

Advantages of Microslice Hyperspectral Imagers Rapid survey speeds with options for multiple viewing geometries. High spatial resolution with no limitations due to scanning speed on a single overpass as with pushbroom techniques. High spectral and spatial resolutions. Longer exposures in stare-mode to allow higher SNR in finer pixels for radiometry, meteorology and atmospheric composition studies. Signal strength is also particularly important for low reflectivity targets such as water and shallow marine environments. Compact design using state-of-the-art sensors to reduce mass/volume requirements.

Summary Knowledge transfer from astronomy to remote sensing is opening up new concepts for hyperspectral imaging of the environment. Extreme multiplex microslice technologies offer a new approach to obtain high spatial and spectral resolution simultaneously over a 2D FoV. The use of step and stare modes offer the potential for 2-3 orders of magnitude increase in S/N compared with pushbroom or whiskbroom approaches and also allows monitoring of time-dependent processes. Further Details: Prof. Ray Sharples - Prof. Danny Donoghue -