Примери за използване на Infrared spectrometer на Английски и техните преводи на Български
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Composite infrared spectrometer.
Infrared spectrometers for breath analysis must comply with the following specifications.
Measuring principle: double wave dispersive infrared spectrometer(NDIR).
Infrared spectrometers for breath analysis must comply with the following specifications.
Using imported German double non dispersive infrared spectrometer(NDIR) sensor based on.
As on Mars 1, an infrared spectrometer was installed to search for signs of methane on Mars.
The spacecraft instrumentation includes a framing camera,a visual and infrared spectrometer, and a gamma-ray and neutron detector.
A semi-automatic sample inlet system injects the measuring gas in definite amounts into the zero gas circulating in the gas circuit of the infrared spectrometer.
Color filters enhance details invisible to human eyes… and an infrared spectrometer scans for minerals that may have formed in the presence of water.
Its properties were revealed in detail by Cassini, which observed it in multiple wavelengths, from the ultraviolet to the infrared, using instruments including its Composite Infrared Spectrometer(CIRS).
While orbiting, the craft's onboard Imaging Infrared Spectrometer will begin searching for the signatures and relative abundance of hydroxyl ions and water molecules.
Strobel, who studies the upper atmospheres of Saturn and Titan,analyzed data from Cassini's composite infrared spectrometer and ion and neutral mass spectrometer in his new paper.
The data were obtained by the composite infrared spectrometer(CIRS) on the Cassini spacecraft during the spacecraft's closest-ever look at Mimas on Feb. 13, 2010.
Strobel, who studies the upper atmospheres of Saturn andTitan, analyzed data from Cassini's composite infrared spectrometer and ion and neutral mass spectrometer in his new paper.
Scientists working with the composite infrared spectrometer, which mapped Mimas' temperatures, expected smoothly varying temperatures peaking in the early afternoon near the equator.
The findings, published February 1 in Icarus, were made using the Composite Infrared Spectrometer(CIRS) on NASA's Cassini spacecraft.
Data from Cassini's composite infrared spectrometer of Enceladus' south polar terrain indicate that the internal heat-generated power is about 15.8 gigawatts, approximately 2.6 times the power output of all the hot springs in the Yellowstone region, or comparable to 20 coal-fueled power stations.
The instruments of the orbiter consisted of two vidicon cameras for imaging(VIS), an infrared spectrometer for water vapor mapping(MAWD) and infrared radiometers for thermal mapping(IRTM).
Data from Cassini's composite infrared spectrometer of Enceladus' south polar terrain, which is marked by linear fissures, indicate that the internal heat-generated power is about 15.8 gigawatts, approximately 2.6 times the power output of all the hot springs in the Yellowstone region, or comparable to 20 coal-fueled power stations.
During that time, she examined the crater using her Visible and Near Infrared Spectrometer(VNIS), which analyzed the light reflecting the surfaces to determine their chemical composition.
Data used in the study came from the Cassini Ion and Neutral Mass Spectrometer and the Composite Infrared Spectrometer along with data returned in 2005 from the Huygens Probe's gas chromatograph-mass spectrometer as it descended via parachute to Titan's surface.
Visual and Infrared Mapping Spectrometer VIMS.
The Nicolet iN10 MX Micro Infrared Imaging Spectrometer.
Geological Survey in Denver,examines data from Cassini's visual and infrared mapping spectrometer.
Cassini's visual and infrared mapping spectrometer has imaged a huge cloud system covering the north pole of Titan.
These images, from Dawn's visible and infrared mapping spectrometer(VIR), highlight two regions on Ceres containing bright spots.
The measurements were made from the NASA Cassini spacecraft using the Visual and Infrared Mapping Spectrometer(VIMS) over the course of the mission.
Cassini's Visual and Infrared Mapping Spectrometer(VIMS) has detected what appears to be a massive ethane cloud surrounding Titan's north pole.
The measurements were made from NASA's Cassini spacecraft by astronomers using its Visual and Infrared Mapping Spectrometer(VIMS) over the course of the mission.
The measurements were made from the NASA-ESA-ASI Cassini spacecraft using the Visual and Infrared Mapping Spectrometer(VIMS), provided by ASI, over the course of the mission.