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D1L4 - Caetano MERIS · MERIS is a programmable, medium-spectral resolution, imaging spectrometer...

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MERIS instrument Mário Caetano June 29th, 2009, D1L4
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Page 1: D1L4 - Caetano MERIS · MERIS is a programmable, medium-spectral resolution, imaging spectrometer operating in the solar reflective spectral range. Fifteen spectral bands can be selected

MERIS instrument

Mário Caetano

June 29th, 2009, D1L4

Page 2: D1L4 - Caetano MERIS · MERIS is a programmable, medium-spectral resolution, imaging spectrometer operating in the solar reflective spectral range. Fifteen spectral bands can be selected

ENVISATMISSION

Page 3: D1L4 - Caetano MERIS · MERIS is a programmable, medium-spectral resolution, imaging spectrometer operating in the solar reflective spectral range. Fifteen spectral bands can be selected

MERIS is a programmable, medium-spectral resolution, imagingspectrometer operating in the solar reflective spectral range. Fifteenspectral bands can be selected by ground command, in the range 390 nm to 1040 nm (bandwidth programmable between 2.5 and 30 nm).

The instrument scans the Earth's surface by the so called "push-broom" method. Linear CCD arrays provide spatial sampling in theacross-track direction, while the satellite's motion provides scanning in the along-track direction.

MERIS is designed so that it can acquire data over the Earth whenever illumination conditions are suitable. The instrument's 68.5° field of view around nadir covers a swath width of 1150 km. This wide field of view is shared between five identical optical modules arranged in a fan shape configuration, providing global coverage every 3 days.

Full resolution: 260m x 300mReduced resolution: 1040m x 1200 m (on-board spatial degradation)

MERIS (MEdium Resolution Image Spectrometer) Instrument

Page 4: D1L4 - Caetano MERIS · MERIS is a programmable, medium-spectral resolution, imaging spectrometer operating in the solar reflective spectral range. Fifteen spectral bands can be selected

ENVISAT

MERIS

Page 5: D1L4 - Caetano MERIS · MERIS is a programmable, medium-spectral resolution, imaging spectrometer operating in the solar reflective spectral range. Fifteen spectral bands can be selected

global coverageevery 3 days

Page 6: D1L4 - Caetano MERIS · MERIS is a programmable, medium-spectral resolution, imaging spectrometer operating in the solar reflective spectral range. Fifteen spectral bands can be selected
Page 7: D1L4 - Caetano MERIS · MERIS is a programmable, medium-spectral resolution, imaging spectrometer operating in the solar reflective spectral range. Fifteen spectral bands can be selected
Page 8: D1L4 - Caetano MERIS · MERIS is a programmable, medium-spectral resolution, imaging spectrometer operating in the solar reflective spectral range. Fifteen spectral bands can be selected
Page 9: D1L4 - Caetano MERIS · MERIS is a programmable, medium-spectral resolution, imaging spectrometer operating in the solar reflective spectral range. Fifteen spectral bands can be selected
Page 10: D1L4 - Caetano MERIS · MERIS is a programmable, medium-spectral resolution, imaging spectrometer operating in the solar reflective spectral range. Fifteen spectral bands can be selected

ON-BOARD CALIBRATION

Page 11: D1L4 - Caetano MERIS · MERIS is a programmable, medium-spectral resolution, imaging spectrometer operating in the solar reflective spectral range. Fifteen spectral bands can be selected
Page 12: D1L4 - Caetano MERIS · MERIS is a programmable, medium-spectral resolution, imaging spectrometer operating in the solar reflective spectral range. Fifteen spectral bands can be selected
Page 13: D1L4 - Caetano MERIS · MERIS is a programmable, medium-spectral resolution, imaging spectrometer operating in the solar reflective spectral range. Fifteen spectral bands can be selected
Page 14: D1L4 - Caetano MERIS · MERIS is a programmable, medium-spectral resolution, imaging spectrometer operating in the solar reflective spectral range. Fifteen spectral bands can be selected

High dynamicrange due tooptimised electronicsallows tomeasure bothvery lowsignals (ocean) and very brightsignals (clouds)

Page 15: D1L4 - Caetano MERIS · MERIS is a programmable, medium-spectral resolution, imaging spectrometer operating in the solar reflective spectral range. Fifteen spectral bands can be selected
Page 16: D1L4 - Caetano MERIS · MERIS is a programmable, medium-spectral resolution, imaging spectrometer operating in the solar reflective spectral range. Fifteen spectral bands can be selected

1 2 3 4 5 6 7 8 9 10 12 1314

Page 17: D1L4 - Caetano MERIS · MERIS is a programmable, medium-spectral resolution, imaging spectrometer operating in the solar reflective spectral range. Fifteen spectral bands can be selected

wavelength (μm) wavelength (μm)

Band 1:Yellow substance, turbidity

Band 2:Chlorophyll absorption maximum

Over land, for atmospheric corrections (blue bands for aerosols retrievals)

Page 18: D1L4 - Caetano MERIS · MERIS is a programmable, medium-spectral resolution, imaging spectrometer operating in the solar reflective spectral range. Fifteen spectral bands can be selected

Band 3:Chlorophyll, other pigments

Band 4:Turbidity, suspended sediment, red tides

Band 5:Chlorophyll reference, suspended sediment

35

Page 19: D1L4 - Caetano MERIS · MERIS is a programmable, medium-spectral resolution, imaging spectrometer operating in the solar reflective spectral range. Fifteen spectral bands can be selected

9

6

Bands 6:9 Chlorophyll absorption, red-edge

Page 20: D1L4 - Caetano MERIS · MERIS is a programmable, medium-spectral resolution, imaging spectrometer operating in the solar reflective spectral range. Fifteen spectral bands can be selected

Band 11 is dedicated to the determination of surface pressure, foraccurate atmospheric corrections (Rayleigh scattering)Uses band 10 as reference baseline.

Page 21: D1L4 - Caetano MERIS · MERIS is a programmable, medium-spectral resolution, imaging spectrometer operating in the solar reflective spectral range. Fifteen spectral bands can be selected

Ratio B11/B10gives at the first orderthe surface pressuredriven by topography

Page 22: D1L4 - Caetano MERIS · MERIS is a programmable, medium-spectral resolution, imaging spectrometer operating in the solar reflective spectral range. Fifteen spectral bands can be selected

MERIS SpectralCalibration Campaigns15 narrow bands(covering the O2-Aabsorption feature)

Page 23: D1L4 - Caetano MERIS · MERIS is a programmable, medium-spectral resolution, imaging spectrometer operating in the solar reflective spectral range. Fifteen spectral bands can be selected

5 cameras varying channel center wavelengths Different impact on bands inside and outside O2-A

Page 24: D1L4 - Caetano MERIS · MERIS is a programmable, medium-spectral resolution, imaging spectrometer operating in the solar reflective spectral range. Fifteen spectral bands can be selected

Band 12:Aerosols, vegetation

Band 13:Aerosols corrections over ocean

Page 25: D1L4 - Caetano MERIS · MERIS is a programmable, medium-spectral resolution, imaging spectrometer operating in the solar reflective spectral range. Fifteen spectral bands can be selected

13 14

15

atmospheric water vapour retrieval

Page 26: D1L4 - Caetano MERIS · MERIS is a programmable, medium-spectral resolution, imaging spectrometer operating in the solar reflective spectral range. Fifteen spectral bands can be selected

MERIS - 14 July 2003 Landsat - 15 July 2003

Page 27: D1L4 - Caetano MERIS · MERIS is a programmable, medium-spectral resolution, imaging spectrometer operating in the solar reflective spectral range. Fifteen spectral bands can be selected
Page 28: D1L4 - Caetano MERIS · MERIS is a programmable, medium-spectral resolution, imaging spectrometer operating in the solar reflective spectral range. Fifteen spectral bands can be selected

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