The spectrometer of NIMS used a grating to disperse the light collected by the telescope.

Parts of a mass spectrometer A mass spectrometer consists of three components an ion source, a mass analyzer, and a detector.

Both the UVS and EUV instruments used a ruled grating to disperse this light for spectral analysis.

MCS (spectrometer) The Mars Climate Sounder (MCS) is a spectrometer with one visible near infrared channel (0.3 to 3.0 μm) and eight far infrared (12 to 50 μm) channels.

The production is beset with difficulties in capturing sound, but by far the worst problem is Lina's grating voice.

In it, she stands with her co star, Tom Ewell, while the air from a subway grating blows her skirt up.

It was particularly grating being subordinated to Paulino Soares and Eusébio de Queirós, protégés whom Honório Hermeto had advanced during the 1830s.

This method employed devices known as calutrons, a hybrid of the standard laboratory mass spectrometer and cyclotron.

As on Mars 1, an infrared spectrometer was installed to search for signs of methane on Mars.

It was made by using a crude version of an instrument we now term as a mass spectrometer.

He is tasked with pushing the specimen into the scanning beam of the Anti Mass Spectrometer for analysis.

An x ray spectrometer, an x ray telescope, cosmic ray detectors, and a laser device were also included.

The spacecraft instrumentation includes a framing camera, a visual and infrared spectrometer, and a gamma ray and neutron detector.

It was detected by the Galileo Near Infrared Mapping Spectrometer (NIMS) from its absorption feature near the wavelength 4.2 micrometers.

The spectrometer observed absorption lines common to hydroxyl, in reflected sunlight, providing evidence of large quantities of water ice, on the lunar surface.

Thermal and evolved gas analyzer The Thermal and Evolved Gas Analyzer (TEGA) is a combination of a high temperature furnace with a mass spectrometer.

Near Infrared Mapping Spectrometer (NIMS) The NIMS instrument was sensitive to 0.7 to 5.2 micrometre wavelength IR light, overlapping the wavelength range of the SSI.

GRO science instruments were Burst and Transient Source Experiment (BATSE), Imaging Compton Telescope (COMPTEL), Energetic Gamma Ray Experiment Telescope (EGRET) and Oriented Scintillation Spectrometer Experiment (OSSE).

Visible and Infrared Mineralogical Mapping Spectrometer (OMEGA)(Observatoire pour la Minéralogie, l'Eau, les Glaces et l'Activité) France Determines mineral composition of the surface up to 100 m resolution.

The first measurements with the Tunable Laser Spectrometer (TLS) indicated that there is less than 5 ppb of methane at the landing site at the point of the measurement.

Both Venera 13 and 14 analysed soil samples with an on board X ray fluorescence spectrometer, and attempted to measure the compressibility of the soil with an impact probe.

However, as soon as the specimen enters the beam, the spectrometer explodes, creating a sudden catastrophe called a resonance cascade , and opening a portal between Earth and a dimension called Xen.

In 1998, the neutron spectrometer located on the Lunar Prospector spacecraft, indicated that high concentrations of hydrogen are present in the first meter of depth in the regolith near the polar regions.

The spacecraft was equipped with four primary science instruments the Contour Remote Imager Spectrograph (CRISP), the Contour Aft Imager (CAI), the Dust Analyzer (CIDA), and the Neutral Gas Ion Mass Spectrometer (NGIMS).

However de Sitter noted that emitter theory predicted several optical effects that were not seen in observations of binary stars in which the light from the two stars could be measured in a spectrometer.

The duty cycle of IMS (the time over which the experiment takes place) is longer than most mass spectrometric techniques, such that the mass spectrometer can sample along the course of the IMS separation.

Alpha Particle X Ray Spectrometer (APXS), developed by the Max Planck Institute for Chemistry in Mainz, Germany, is used for close up analysis of the abundances of elements that make up rocks and soils.

It carried 10 experiments to study formation of metal alloys in microgravity, the operation of heat pipes, instruments for remote sensing observations, and a mass spectrometer to identify various gases in the payload bay.

MERIS 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.

During the week of February 20, 2006, controllers conducted initial in flight tests of three onboard science instruments, the Alice ultraviolet imaging spectrometer, the PEPSSI plasma sensor, and the LORRI long range visible spectrum camera.

The final stages, when I ran the samples through a high pressure liquid chromatography mass spectrometer, which separated the compounds and analyzed the chemicals and told me exactly how much carcinogens I had in my chicken.

To accomplish these goals, the spacecraft was equipped with an X ray gamma ray spectrometer, a near infrared imaging spectrograph, a multi spectral camera fitted with a CCD imaging detector, a laser rangefinder, and a magnetometer.

IRS (Infrared Spectrograph), an infrared spectrometer with four sub modules which operate at the wavelengths 5.3 14 µm (low resolution), 10 19.5 µm (high resolution), 14 40 µm (low resolution), and 19 37 µm (high resolution).

MIPAS 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 (), nitrous oxide (), methane (), nitric acid (), ozone (), and water () in the stratosphere.

Servicing Mission 2 Servicing Mission 2, flown by Discovery in February 1997, replaced the GHRS and the FOS with the Space Telescope Imaging Spectrograph (STIS) and the Near Infrared Camera and Multi Object Spectrometer (NICMOS), replaced an Engineering and Science Tape Recorder with a new Solid State Recorder, and repaired thermal insulation.

A strong burst could result in the observation of many thousands of gamma rays within a time interval ranging from 0.1 s up to about 100 s. OSSE The Oriented Scintillation Spectrometer Experiment, (OSSE), by the Naval Research Laboratory detected gamma rays entering the field of view of any of four detector modules, which could be pointed individually, and were effective in the 0.05 to 10 MeV range.