Model of Envisat |
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Operator | European Space Agency |
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Mission type | Earth observation |
Launch date | 1 March 2002 at 01:07 UTC |
Carrier rocket | Ariane 5 |
COSPAR ID | 2002-009A |
Homepage | http://envisat.esa.int/ envisat.esa.int |
Mass | 8,211 kg (18,100 lb) |
Orbital elements | |
Regime | Polar orbit |
Inclination | 98.6° |
Apoapsis | 791 km (492 mi) |
Periapsis | 785 km (488 mi) |
Orbital period | 100.6 min |
Repeat interval | 35 days |
Instruments | |
ASAR RA-2 MWR MIPAS |
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Main instruments | MERIS AATSR DORIS GOMOS SCIAMACHY |
Envisat ("Environmental Satellite") is an Earth-observing satellite. It was launched on 1 March 2002 aboard an Ariane 5 from the Guyana Space Centre in Kourou, French Guyana into a Sun synchronous polar orbit at an altitude of 790 km (490 mi) (± 10 km (6.2 mi)). It orbits the Earth in about 101 minutes with a repeat cycle of 35 days.
This €2.3 billion European Space Agency (ESA) programme launched the largest earth observation satellite put into space (as of late 2006), being 26 m (85 ft) × 10 m (33 ft) × 5 m (16 ft) and having a mass of 8.5 t (8.4 long tons; 9.4 short tons).
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Envisat is an Earth observation satellite. Its objective is to service the continuity of European Remote-Sensing Satellite missions, providing additional observational parameters to improve environmental studies.
In working towards the global and regional objectives of the mission, numerous scientific disciplines use the data acquired from the different sensors on the satellite, to study such things as atmospheric chemistry, ozone depletion, biological oceanography, ocean temperature and colour, wind waves, hydrology (humidity, floods), agriculture and arboriculture, natural hazards, digital elevation modelling (using interferometry), monitoring of maritime traffic, atmospheric dispersion modelling (pollution), cartography and study of snow and ice.
Envisat carries an array of nine Earth-observation instruments that gather information about the earth (land, water, ice, and atmosphere) using a variety of measurement principles. A tenth instrument, DORIS, provides guidance and control.
Several of the instruments are advanced versions of instruments that were flown on the earlier ERS 1 and ERS 2 missions and other satellites.
MERIS (MEdium Resolution Imaging Spectrometer) measures the reflectance of the Earth (surface and atmosphere) in the solar spectral range (390 to 1040 nm) and transmits 15 spectral bands back to the ground segment.
MERIS was built at the Cannes Mandelieu Space Center.
AATSR (Advanced Along Track Scanning Radiometer) can measure the temperature of the sea surface.
It is a passive radiometer which aims to measure the tempemissions from the surface of the earth in the visible and infrared spectra. Because of its wide angle lens it is possible to make very precise measurements of atmospheric effects on how emissions from the Earth's surface propagate.
AATSR is the successor of ATSR1 and ATSR2, payloads of ERS 1 and ERS 2. AATSR can measure Earth's surface temperature to a precision of 0.3 K (0.54 °F), for climate research.
Among the secondary objectives of AATSR is the observation of environmental parameters such as water content, biomass, and vegetal health and growth.
GOMOS (Global Ozone Monitoring by Occultation of Stars) uses the principle of occultation. Its sensors detect light from a star traversing the Earth's atmosphere and measures the depletion of that light by trace gases nitrogen dioxide (NO2), nitrogen trioxide, (NO3), OClO), ozone (O3) and aerosols present between about 20 to 80 km (12 to 50 mi) altitude. It has a resolution of 3 km (1.9 mi).
SCIAMACHY (SCanning Imaging Absorption spectroMeter for Atmospheric CHartographY) compares light coming from the sun to light reflected by the Earth, which provides information on the atmosphere through which the earth-reflected light has passed.
SCIAMACHY is an image spectrometer with the principal objective of mapping the concentration of trace gases and aerosols in the troposphere and stratosphere. Rays of sunlight that are reflected transmitted, backscattered and reflected by the atmosphere are captured at a high spectral resolution (0.2 to 0.5 nm) for wavelengths between 240 to 1,700 nm, and in certain spectra between 2,000 and 2,400 nm.
Its high spectral resolution over a wide range of wavelengths can detect many trace gases even in tiny concentrations. The wavelengths captured also allow effective detection of aerosols and clouds.
SCIAMACHY uses 3 different targeting modes: to the nadir (against the sun), to the limbus (through the atmospheric corona), and during solar or lunar eclipses.
RA-2 (Radar Altimeter 2) is a dual-frequency Nadir pointing Radar operating in the Ku band and S bands, it is used to define ocean topography, map/monitor sea ice and measure land heights.
One interesting aspect of the mission is the low rate of global mean sea level rise which it has measured over the first eight years of the mission: just 0.5 mm/year, which is about 1/4 the rate of GMSL rise measured over the same period by the Jason-1 satellite. Mean sea level measurements from Envisat are continuously graphed at the Centre National d'Etudes Spatiales web site, on the Aviso page.
MWR (Microwave Radiometer) for measuring water vapour in the atmosphere and estimate the tropospheric delay for the Altimeter
DORIS (Doppler Orbitography and Radiopositioning Integrated by Satellite) determines the satellite's orbit to within 10 centimetres (4 in).
GOMOS (Global Ozone Monitoring by Occultation of Stars) looks to stars as they descend through the Earth's atmosphere and change color, which also tells a lot about the presence of gases such as ozone (O3), and allows for the first time a space-based measurement of the vertical distribution of these trace gases.
MIPAS (Michelson Interferometer for Passive Atmospheric Sounding) is a Fourier transforming infrared spectrometer which provides pressure and temperature profiles, and profiles of trace gases nitrogen dioxide (NO2), nitrous oxide (N2O), methane (CH4), nitric acid (HNO3), ozone (O3), and water (H2O) in the stratosphere. The instrument functions with high spectral resolution in an extended spectral band, which allows coverage across the globe in all seasons and at equal quality night and day. MIPAS has a vertical resolution of 3 to 5 kilometres (2 to 3 mi) depending on altitude (the larger at the level of the upper stratosphere).
ASAR (Advanced Synthetic Aperture Radar) operates in the C band in a wide variety of modes. It can detect changes in surface heights with sub-millimeter precision. It serves as a data link for ERS 1 and ERS 2, providing numerous functions such as observations of different polarities of light or combining different polarities, angles of incidence and spatial resolutions.
Mode | Id | Polarisation | Incidence | Resolution | Swath |
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Alternating polarisation | AP | HH/VV, HH/HV, VV/VH | 15 – 45° | 30 – 150 m | 58 – 110 km |
Image | IM | HH, VV | 15 – 45° | 30 – 150 m | 58 – 110 km |
Wave | WV | HH, VV | 400 m | 5 × 5 km | |
Suivi global (ScanSAR) | GM | HH, VV | 1 km | 405 km | |
Wavescan (ScanSAR) | WS | HH, VV | 150 m | 405 km |
These different types of raw data can be given several levels of treatment (suffixed to the ID of the acquisition mode: IMP, APS, and so on):
Data capture in WV mode is unusual in that they constitute a series of 5 km × 5 km spaced at 100 km.
Envisat cost 2.3 BEuro (including 300 MEuro for 5 years operations) to develop and launch [1]
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