Medium Resolution Imaging Spectrometer (MERIS)

Source:http://www.naturalsciences.be	Source: http://mtp.jpl.nasa.gov

MERIS is a programmable, medium-spectral resolution, imaging spectrometer operating in the solar reflective spectral range. Fifteen spectral bands can be selected by ground command. The instrument scans the Earth's surface by the so called "push-broom" method. Linear CCD arrays provide spatial sampling in the across-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. MERIS coverage for the SMAPEx study area is summarised in the table below. MERIS data can be downloaded from ESA.

Mission	MERIS
Sensor	Medium Resolution Imaging Spectrometer (MERIS)
Spacecraft	Envisat
Launch date	1st, Mar. 2002
Design life	3 years with a goal of 5 years
Orbit	Sun-synchronous polar orbit (SSO): Nominal reference orbit of mean altitude 800km, 35 days repeat cycle, 10:00am mean local solar time (MLST) descending node, 98.55°. inclination. [envisat.esa.int]
Spacecraft operations control centre	ESA
Accuracy	Ocean colour bands typical S:N = 1700
Swath (km)	1150
Waveband	VIS-NIR: 15 bands selectable across range: 390 nm to 1040 nm (bandwidth programmable between 2.5 and 30 nm)
Spatial resolution (m)	Ocean: 1040m x 1200 m, Land & coast: 260m x 300m
Temporal resolution	35 days repeat cycle