For example, one of the mission's instruments called the Mapping
Imaging Spectrometer for Europa (MISE) will identify and map the amount of possible life - giving elements like organic material, salts, and acid hydrates in Europa's surface and underwater ocean.
A split
imaging spectrometer for temporally and spatially resolved titanium absorption spectroscopy
Once he had the signal from the lab glass, he used an algorithm designed to pick out similar signals in data from the Compact Reconnaissance
Imaging Spectrometer for Mars (CRISM), which flies aboard NASA's Mars Reconnaissance Orbiter.
Detection of the impact glass by researchers at Brown University, Providence, R.I., is based on data from the Compact Reconnaissance
Imaging Spectrometer for Mars (CRISM) on NASA's Mars Reconnaissance Orbiter.
Regolith X-ray
Imaging Spectrometer (REXIS)-- A student experiment provided by the Massachusetts Institute of Technology (MIT) and Harvard University in Cambridge, which will observe the X-ray spectrum to identify chemical elements on Bennu's surface and their abundances.
Examination of some of the scarps with MRO's Compact Reconnaissance
Imaging Spectrometer for Mars (CRISM) confirmed that the bright material is frozen water.
Using
an imaging spectrometer on MRO, researchers detected signatures of hydrated minerals on slopes where mysterious streaks are seen on the Red Planet.
Using a unique, high - fidelity
imaging spectrometer onboard the Carnegie Airborne Observatory, Asner and his team made the first - ever forest canopy maps of leaf nitrogen, phosphorus, and mass over a large portion of the biosphere covering nearly 200 million acres of Peru.
The new study pairs HiRISE observations with mineral mapping by MRO's Compact Reconnaissance
Imaging Spectrometer for Mars (CRISM).
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.
Images from Cassini's ultraviolet
imaging spectrometer (UVIS), obtained from an unusually close range of about six Saturn radii, provided a look at the changing patterns of faint emissions on scales of a few hundred miles (kilometers) and tied the changes in the auroras to the fluctuating wind of charged particles blowing off the sun and flowing past Saturn.
Intense extreme ultraviolet FEL pulses were directed at the clusters and the resultant energy distribution of electrons knocked out of the clusters was measured using a «velocity map
imaging spectrometer».
Then the larger research team used data from the sensor onboard the European Space Agency's Envisat satellite MEdium Resolution
Imaging Spectrometer (MERIS) to examine how the color of the lake water changed during those years — an indication of the concentration of the toxic blue - green algae present in HABs.
That's the job of the Complex Reconnaissance
Imaging Spectrometer for Mars, or CRISM.
Working with the Canadian Space Agency, GHGSat spent three years designing a satellite whose lightweight
imaging spectrometer can focus on an area as small as 164 square feet.
The telescope, which recently lost one of its four main instruments,
the imaging spectrometer, could fail as early as 2007 without new batteries.
An international team of 32 authors from 24 institutions in eight countries led the effort, which involved using satellite data from NASA's Moderate Resolution
Imaging Spectrometer and the National Oceanic and Atmospheric Administration's Advanced Very High Resolution Radiometer instruments to help determine the leaf area index, or amount of leaf cover, over the planet's vegetated regions.
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.
Now, a team using
an imaging spectrometer aboard NASA's Mars Reconnaissance Orbiter reports the discovery of numerous patches of opaline silica across the Red Planet.
The Compact
Imaging Spectrometer for Mars (CRISM) observed comet C / 2013 A1 Siding Spring as the comet sped close to Mars on Oct. 19.
The data were gathered using the Advanced CCD
Imaging Spectrometer on Chandra, an instrument conceived and designed by a team led by Penn State Evan Pugh Professor Emeritus of Astronomy and Astrophysics Gordon Garmire.
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.
Due to launch on Aug. 8, 2013, the VERIS rocket, short for Very high Resolution
Imaging Spectrometer, will launch for a 15 - minute trip carrying an instrument that can measure properties of the structures in the sun's upper atmosphere down to 145 miles across, some eight times clearer than any similar telescope currently in space.
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 hemisphere.
The Low Resolution
Imaging Spectrometer (LRIS) is a very versatile visible - wavelength imaging and spectroscopy instrument commissioned in 1993 and operating at the Cassegrain focus of Keck I.
The space agency says that the MRO watched the comet go by with its High Resolution Imaging Science Experiment (HiRISE), the Compact
Imaging Spectrometer for Mars (CRISM), and the Context Camera (CTX), and will continue to observe the comet while it remains within range over the next few days.
Image from the Compact Reconnaissance
Imaging Spectrometer for Mars (CRISM) instrument on the Mars Reconnaissance Orbiter, showing deposits of impact glass (green) in Alga Crater.
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).
During this period, in - flight tests were conducted on the spacecraft's Alice ultraviolet
imaging spectrometer and Pluto Energetic Particle Spectrometer Science Investigation (PEPSSI), as well as LORRI, and New Horizons passed the orbit of Mars in April 2006.
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).
«Having global access with modern
imaging spectrometers from lunar orbit is the next best thing to having a geologist with a rock hammer doing the field work across the surface.»
During the past five years, researchers used OMEGA and NASA's Compact Reconnaissance
Imaging Spectrometer, or CRISM, instrument on the Mars Reconnaissance Orbiter to identify clay minerals at thousands of locations on Mars.
The distance to the quasar is so great (about 10 billion light - years) that the emitted light is «stretched» by the expansion of the universe from an invisible ultraviolet wavelength to a visible shade of violet by the time it reaches the 10 - meter Keck I telescope and the LRIS (Low Resolution
Imaging Spectrometer) used for this discovery.
As New Horizons glides behind Pluto and its shadow during the flyby, an ultraviolet
imaging spectrometer aboard the spacecraft, named Alice, will analyze the filtered sunlight that passes through Pluto's atmosphere.
When New Horizons arrives at the Pluto system, onboard science instruments such as Alice, a sensitive ultraviolet
imaging spectrometer, will reveal even more about the composition and structure of the dwarf planet's dynamic atmosphere.
Abstract: Using the Chandra Advanced CCD
Imaging Spectrometer Imaging array (ACIS - I), we have carried out a deep hard X-ray observation of the Galactic plane region at (l, b) ~ (28.5, 0.0), where no discrete X-ray source had been reported previously.
Alice is an ultraviolet
imaging spectrometer whose purpose is to study the atmospheric structure and composition of Pluto.
Seen at the top left, the Chandra X-ray Observatory's false color view of the Cartwheel galaxy was taken with the S - array on the telescope's Advanced CCD
Imaging Spectrometer.
At the global scale, outgoing LW flux anomalies are partially compensated for by decreases in mid latitude cloud fraction and cloud height, as observed by Moderate Resolution
Imaging Spectrometer and Multi-angle Imaging Spectro Radiometer, respectively.
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.
Lower - resolution sensors such as the Moderate Resolution Imaging Spectroradiometer (MODIS) and Medium Resolution
Imaging Spectrometer (MERIS) have also been effective in estimating ZSD in estuaries and offshore marine waters.
We just received approval from NASA Headquarters to fly the Airborne Visible / Infrared
Imaging Spectrometer (AVIRIS) over these fires.
An international team of 32 authors from 24 institutions in eight countries led the effort, which involved using satellite data from NASA's Moderate Resolution
Imaging Spectrometer and the National Oceanic and Atmospheric Administration's Advanced Very High Resolution Radiometer instruments to help determine the leaf area index, or amount of leaf cover, over the planet's vegetated regions.
Not exact matches
Further detectors inside the tank look for decay particles: a magnetic
spectrometer measures the momentum of charged tracks from kaon decays, a ring
imaging Cherenkov (RICH) detector tells the team the nature of decay particles, and electromagnetic and hadronic calorimeters measure their energy.
For Huygens's crucial
imaging camera and
spectrometer, the channel A mishap touched off a different set of troubles.
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.
In another study, the craft used its Fast
Imaging Plasma
Spectrometer to identify energetic charged atoms and molecules (plasma) caught in Mercury's magnetic field.
Chemical
imaging involves the use of a laser or ion beam to analyse the sections of skin using a mass
spectrometer.