We just received approval from NASA Headquarters to fly the Airborne Visible /
Infrared Imaging Spectrometer (AVIRIS) over these fires.
Infrared Imaging Spectrometer (IRIS) The
Infrared Imaging Spectrometer (IRIS) will be mounted on the observatory Adaptive Optics system and be capable of diffraction - limited imaging and integral - field spectroscopy at near - infrared wavelengths (0.8 — 2.5 μm).
It consists of a charge - coupled device camera with four color filters spanning wavelengths from 400 to 970 nm plus a near -
infrared imaging spectrometer covering wavelengths from 1.25 to 2.5 μm, where the various cryogenic ices are distinguishable via their characteristic vibrational absorption features.
Not exact matches
This study used variations in the thermal emissivity of the surface observed by the Visible and
Infrared Thermal
Imaging Spectrometer on the European Space Agency's Venus Express spacecraft to identify compositional differences in lava flows at three hotspots.
Orbiting instruments like the Moderate Resolution
Imaging Spectrometer on the Aqua satellite, and the Visible
Infrared Imaging Radiometer Suite on the Suomi NPP satellite collect data on the color of the ocean.
And until now, Cassini's visual and
infrared mapping
spectrometer and
imaging science subsystem had only been able to capture distant, oblique or partial views of this area.
The Visible and
Infrared Thermal Imaging Spectrometer (VIRTIS) instrument captured this infrared radiation during Venus Express's night - time orbits around the planet's southern hem
Infrared Thermal
Imaging Spectrometer (VIRTIS) instrument captured this
infrared radiation during Venus Express's night - time orbits around the planet's southern hem
infrared radiation during Venus Express's night - time orbits around the planet's southern hemisphere.
Infrared Multi-object Spectrometer (IRMS) The Infrared Multi-object Spectrometer (IRMS) will allow close to diffraction - limited imaging and slit spectroscopy over a 2 arcminute diameter field - of - view at near - infrared wavelengths (0.8 —
Infrared Multi-object
Spectrometer (IRMS) The
Infrared Multi-object Spectrometer (IRMS) will allow close to diffraction - limited imaging and slit spectroscopy over a 2 arcminute diameter field - of - view at near - infrared wavelengths (0.8 —
Infrared Multi-object
Spectrometer (IRMS) will allow close to diffraction - limited
imaging and slit spectroscopy over a 2 arcminute diameter field - of - view at near -
infrared wavelengths (0.8 —
infrared wavelengths (0.8 — 2.5 μm).
In addition, MSSS built the Mars Odyssey (ODY) Thermal Emission
Imaging Spectrometer (THEMIS) Visible (VIS) camera subsystem, which shares optics with the thermal
infrared instrument and is operated at Arizona State University (ASU).
The Near
Infrared Camera and Multi-Object Spectrometer (NICMOS) is an HST instrument providing the capability for infrared imaging and spectroscopic observations of astronomical
Infrared Camera and Multi-Object
Spectrometer (NICMOS) is an HST instrument providing the capability for
infrared imaging and spectroscopic observations of astronomical
infrared imaging and spectroscopic observations of astronomical targets.
This view combines the sharp
imaging of the Hubble Space Telescope's Near
Infrared Camera and Multi-Object
Spectrometer (NICMOS) with color imagery from a previous Spitzer Space Telescope survey done with its
Infrared Astronomy Camera (IRAC).
The photodetector array camera and
spectrometer (PACS) aboard the Herschel Space Observatory allows
imaging observations in the far
infrared at unprecedented resolution, i.e. at better than 6» to 12» over the wavelength range of 60 -LCB- \ mu -RCB- m to 210 -LCB- \ mu -RCB- m. Together with the results from ground - based observations, these spatially resolved data can be modelled to determine the nature of the debris and its evolution more reliably than would be possible from unresolved data alone.
Sources such as the Tropospheric Emission
Spectrometer (TES), Ozone Monitoring Instrument (OMI), and Moderate Resolution
Imaging Spectroradiometer (MODIS) instruments on the Aura satellite, the Cloud - Aerosol Lidar and
Infrared Pathfinder Satellite Observations (CALIPSO), and the ground - based Aerosol Robotic Network (Aeronet) will be used, requiring the input of both the modeling and observational communities.
Over the ocean this includes: sea surface slope and surface current, significant wave height, wind speed and sea level from radar altimetry at about 10 km resolution: sea surface temperature under cloud free conditions from the
infrared radiometer at about 300 m resolution; chlorophyll a and phytoplankton from the
imaging spectrometer under cloud free conditions at about 300 m resolution.
Over the sea ice field the observations include: sea ice freeboard height and hence sea ice thickness from radar altimetry; sea ice surface temperature and sea ice drift from respectively
infrared radiometer and
imaging spectrometer under cloud free conditions.
The two satellites are in a polar orbit with an inclination of about 82 degrees and operates 3 distinct instruments: a radar altimeter; an
imaging spectrometer; and an
infrared radiometer.