Sentences with phrase «imaging spectrometer for»

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.

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.

The Compact Imaging Spectrometer for Mars (CRISM) observed comet C / 2013 A1 Siding Spring as the comet sped close to Mars on Oct. 19.

That's the job of the Complex Reconnaissance Imaging Spectrometer for Mars, or CRISM.

The new study pairs HiRISE observations with mineral mapping by MRO's Compact Reconnaissance Imaging Spectrometer for Mars (CRISM).

Examination of some of the scarps with MRO's Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) confirmed that the bright material is frozen water.

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.

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.

A split imaging spectrometer for temporally and spatially resolved titanium absorption spectroscopy

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.

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.

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.

Herbert Funsten is recognized as a world - renowned experimental space scientist and has led science instruments on NASA's Interstellar Boundary Explorer (IBEX) and Van Allen Probes missions and national security instruments on the DOE's SABRS Validation Experiment (SAVE) and Space and Atmospheric Burst Reporting System (SABRS) payloads, while also participating in NASA's Cassini, Two Wide - angle Imaging Neutral - atom Spectrometers (TWINS), Deep Space 1, Mars Odyssey, and Imager for Magnetopause - to - Aurora Global Exploration (IMAGE) missions.

The Williams lab also has an imaging time - of - flight secondary ion mass spectrometer used for novel bioimaging applications.

Velten's current work with the medical devices team at the Morgridge Institute for Research focuses on the imaging technology used in advanced microscopes and mass spectrometers.

The Near Infrared Camera and Multi-Object Spectrometer (NICMOS) is an HST instrument providing the capability for infrared imaging and spectroscopic observations of astronomical targets.

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.

The self - assembly occurred in a gas phase, cluster beam condensation source, before size - selection with a mass spectrometer and deposition onto a carbon surface for oxidation and then imaging.

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.

Scientists first noticed the data years ago amid satellite measurements collected by the European Space Agency's (ESA) Scanning Imaging Absorption Spectrometer for Atmospheric Chartography (SCIAMACHY) instrument.