Imaging from Space · 2016. 12. 12. · 1 WE PARTNER WITH OUR CUSTOMERS TO IMPROVE, SAVE AND...

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WE PARTNER WITH OUR CUSTOMERS TO IMPROVE, SAVE AND PROTECT PEOPLE’S LIVES Imaging from Space Paul Jerram Chief Engineer, Space imaging

Transcript of Imaging from Space · 2016. 12. 12. · 1 WE PARTNER WITH OUR CUSTOMERS TO IMPROVE, SAVE AND...

  • 1WE PARTNER WITH OUR CUSTOMERS TO IMPROVE, SAVE AND PROTECT PEOPLE’S LIVES

    Imaging from Space

    Paul JerramChief Engineer, Space imaging

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    Imaging from Space

    Alternative types of sensors and modes of operation – Snapshot imagers• Work like the detector in your camera• Generally not good for Earth Observation– but used for astronomy• Can either be colour or monochrome

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    Imaging from Space

    Alternative types of sensors and modes of operation – Linear Imagers• The simplest type of detector is a linear (one row of pixels). This scans

    the ground like a sensor in a photocopier• Several linear sensors are used together with filters to give a colour

    image• Relatively easy application to switch to CMOS (eg Sentinel 2)

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    Imaging from Space

    Alternative types of sensors and modes of operation – TDI imagers• The operating principle of TDI imagers is similar to linear detector• Push-broom (scanning) operation• Several lines are added together on chip to increase sensitivity• Used for high resolution high sensitivity imaging (eg Pleiades, New

    Horizons)

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    Imaging from Space

    Alternative types of sensors and modes of operation – Hyperspectral imagers• Spectrum is dispersed across a 2D array• Still scans the ground but with high quality spectral information• Normally low spatial resolution but high spectral resolution

    One line from the ground

    Is split into spectral lines

    And imaged as many lines on a detector

    http://www.google.co.uk/url?sa=i&rct=j&q=&esrc=s&source=images&cd=&cad=rja&uact=8&ved=0ahUKEwitxPn6kP3OAhVGXBQKHd0PBKsQjRwIBw&url=http://www.briansolis.com/2014/02/quality-prism-secret-co-creating-brands-social-media/&psig=AFQjCNEyTtZO9xucAwAyXbV6qkW0fV9AOw&ust=1473333453546299

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    e2v inside ESA Sentinel 3A Copyright Contains modified Copernicus Sentinel data [2016]/ processed by ESA

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    Sentinel 2: image from ESA

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    ESA’s Earth Observation Fleet

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    ESA’s Earth Observation Fleet

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    Who would have thought that comets look like this?

    e2v inside ESA RosettaCopyright ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA

    Osiris CCD42-40

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    Or that Pluto would be such a strange world?

    e2v inside NASA New HorizonCopyright NASA/JHUAPL/SwRI

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    Charon

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    Just one of the surprises from Mars

    e2v inside NASA Mars reconnaissance orbiterCopyright BATC NASA

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    e2v inside SDOCopyright Solar Dynamics Observatory/NASA

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    GAIA: Mapping our galaxy with unprecedented precision

  • 21e2v inside KeplerCopyright NASA Ames / W. Stenzel; May 10 2016

    Finding “Earth like “ planets

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    Seeing back to nearly the origins of the Universe13.2 billion light year

    e2v inside Hubble Copyright NASA/STScl

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    Copyright NASA/STScl23

    Hubble

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    ..and the future

    PLATO

    EUCLID

    Many earth observation missions

    LSST

    + many more

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    The e2v 1.2 Giga-pixel camera

    Opto-mechanical subsystem verification

    The focal plane inside the cryostat plane and flatness measurements made at -110 oC showing the 14 science devices, 8 wavefront and 4 autoguide CCDs.

    Flatness achieved - 27 µm peak to valley for (spec 40µm target 30µm)

    Metrology has been developed to make this measurement at operating temperature

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    Channel Number (output)

    1 2 3 45 6 7 89 10 11 1213 14

    Requirement

    633 kHz per output 400 kHz per output

    Noise from all outputs from all devices shown

    All devices and outputs read out in parallelWavefront and Autoguide devices operating

    Target

    Tplate = -110oC

    Device number

    The measured system noise for all devices operating in parallel

    Inter channel and inter device cross talk better than 106 dB

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    e2v is developing a focal plane to study the universe in Ultraviolet

    WSO-UV space mission is to study the Universe in the 120 - 310 nm ultraviolet (UV) wavelengths range, which is beyond the reach of ground-based instruments. .

    3 off Camera Electronics Box

    3 off Cryostaticenclosures housing CCD

    Package (e2v)

    CCD272

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    Thank you for your attention

    Slide Number 1Imaging from SpaceImaging from SpaceImaging from SpaceImaging from SpaceSlide Number 9Slide Number 10Slide Number 11Slide Number 12ESA’s Earth Observation FleetESA’s Earth Observation FleetSlide Number 15Slide Number 16CharonSlide Number 18Slide Number 19Slide Number 20Slide Number 21Slide Number 22�Copyright NASA/STScl..and the futureThe e2v 1.2 Giga-pixel camerae2v is developing a focal plane to study �the universe in UltravioletSlide Number 27