* Passive Infrared Detector, a PIR-based motion detector

However, a new system called Airborne Volcanic Object Infrared Detector ( AVOID ) has recently been developed by Nicarnica Aviation, a daughter company of the Norwegian Institute for Air Research, which will allow pilots to detect ash plumes up to 100 km ( 62 mi ) ahead and fly safely around them.

All carbon present converts to carbon dioxide, flows through scrubber tubes to remove interferences such as chlorine gas, and water vapor, and the carbon dioxide is measured either by absorption into a strong base then weighed, or using an Infrared Detector.

* Infrared Obstacle Detector ( chest array )— used to detect objects for collision avoidance, edge detection.

* Infrared Processing Center, at Oak Ridge National Laboratory

The Infrared Optical Telescope Array ( IOTA ) began with an agreement in 1988 among five Institutions, the Smithsonian Astrophysical Observatory, Harvard University, the University of Massachusetts Amherst, the University of Wyoming, and MIT / Lincoln Laboratory, to build a two-telescope stellar interferometer for the purpose of making fundamental astrophysical observations, and also as a prototype instrument on which we could perfect techniques which could later lead to the development of a larger, more powerful array.

For example, Lowell staff built a sophisticated high-speed camera for use on the Stratospheric Observatory for Infrared Astronomy ( SOFIA ).

The NASA Infrared Telescope Facility ( NASA IRTF ) is a telescope optimized for use in infrared astronomy and located at the Mauna Kea Observatory in Hawai ' i. It was first built to support the Voyager missions and is now the USA national facility for infrared astronomy, providing continued support to planetary, solar neighborhood, and deep space applications.

SpeX is a medium-resolution 0. 8-5. 4 µm spectrograph built at the Institute for Astronomy ( IfA ), for the NASA Infrared Telescope Facility ( IRTF ) on Mauna Kea.

NSFCAM2 is a 1-5 µm camera, built at the Institute for Astronomy, ( IfA ), for the NASA Infrared Telescope Facility ( IRTF ).

The MIRACL Near Infrared Laser, at White Sands Missile Range, NM was fired at a stationary Titan I second stage that was fixed to ground.

; NIRC: The Near Infrared Camera for the Keck I telescope is so sensitive it could detect the equivalent of a single candle flame on the Moon.

; NIRC-2: The second generation Near Infrared Camera works with the Keck Adaptive Optics system to produce the highest-resolution ground-based images and spectroscopy in the 1 – 5 micrometers ( µm ) range.

; NIRSPEC: The Near Infrared Spectrometer studies very high redshift radio galaxies, the motions and types of stars located near the Galactic Center, the nature of brown dwarfs, the nuclear regions of dusty starburst galaxies, active galactic nuclei, interstellar chemistry, stellar physics, and Solar System science.

Radial velocity measurements of this star using the Near Infrared Spectrometer ( NIRSPEC ) instrument at the Keck II observatory have not revealed any variations that might otherwise indicate the presence of an orbiting companion.

* Visible and Near Infrared: 0. 6 μm – 1. 6 μm – For recording cloud cover during the day

For example, the James Webb Space Telescope is, as its name indicates, a telescope, but it includes a suite of four distinct scientific instruments: Mid Infrared Instrument ( MIRI ); Near Infrared Camera ( NIRCam ); Near Infrared Spectrograph ( NIRSpec ); Fine Guidance Sensor Tunable Filter Imager ( FGS-TFI ).

* The Near Infrared Camera / Fabry – Pérot Spectrometer ( NICFPS ) was developed at the University of Colorado.

The two older instruments being replaced were the Goddard High Resolution Spectrograph and the Faint Object Spectrograph, exchanged for the Space Telescope Imaging Spectrograph ( STIS ) and the Near Infrared Camera and Multi-Object Spectrometer ( NICMOS ), respectively.

Lee and Smith removed two scientific instruments from Hubble, the Goddard High Resolution Spectrograph ( GHRS ) and Faint Object Spectrograph ( FOS ), and replaced them with the Space Telescope Imaging Spectrograph ( STIS ) and Near Infrared Camera and Multi-Object Spectrometer ( NICMOS ), respectively.

# REDIRECT Near Field Infrared Experiment

The Near Field Infrared Experiment ( NFIRE ) is a satellite which was proposed and developed by the Missile Defense Agency, a division of the United States Department of Defense.

de: Near Field Infrared Experiment

The crew of STS-109 successfully upgraded the Hubble Space Telescope ’ s systems over the course of five consecutive EVAs, leaving it with a new power control unit, improved solar arrays, the new Advanced Camera for Surveys ( ACS ), and an experimental refrigeration unit for cooling the dormant Near Infrared Camera and Multi-Object Spectrometer ( NICMOS ).

* Near Infrared, infrared radiation of a wavelength near that of red

False-color image of the Pistol Star and Pistol Nebula, taken by Near Infrared Camera and Multi-Object Spectrometer | NICMOS

His dissertation is entitled A Spectrographic Study of the Night Sky and Aurora in the Near Infrared.

* Near Field Infrared Experiment ( NFIRE )

; Multi-Object Infrared Camera and Spectrograph ( MOIRCS ): Wide-field camera and spectrograph with the ability to take spectra of multiple objects simultaneously, mounts on the Cassegrain focus.

; Infrared Camera and Spectrograph ( IRCS ): Used in conjunction with the new 188-element adaptive optics unit ( AO188 ), mounted at the infrared Nasmyth focus.

; Cooled Mid Infrared Camera and Spectrometer ( COMICS ): Mid-infrared camera and spectrometer with the ability to study cool interstellar dust, mounts on the Cassegrain focus.

As of 2011, the engineers are working on the High-resolution Airborne Wideband Camera ( HAWC ), which will be an integral part of Stratospheric Observatory for Infrared Astronomy ( SOFIA ).

This payload consisted of the Cryogenic Infrared Radiance Instrumentation for Shuttle ( CIRRIS-1A ) experiment, Far Ultraviolet Camera experiment ( FAR UV ), the Uniformly Redundant Array ( URA ), the Quadrupole Ion Neutral Mass Spectrometer ( QINMS ), and the Horizon Ultraviolet Program ( HUP ) experiment.

* Infrared Camera ( ISOCAM )-A high-resolution camera covering 2. 5 to 17 micrometre wavelength with two different detectors.

* Sonobuoys, Radar, Wescam MX-20 Electro-Optical / Infrared ( EO / IR ) suite, Magnetic anomaly detector ( MAD ), Electronic Support Measures ( ESM ), Applanix DSS-439 Digital Mapping Camera ( DSS ), hand-held digital camera, gyro-stabilized binoculars, 3 AN / ARC-210 V / UHF Radios, 1 AN / ARC-234 V / UHF SATCOM Radio.

There are two related projects: the Wide Field Camera ( WFCAM ) on the United Kingdom Infrared Telescope in Hawaii carries out infrared surveys of the northern sky, and the VLT Survey Telescope in Chile carries out surveys of the southern sky in visible light.

* NICS (" Near Infrared Camera and Spectrometer "), camera and spectrograph for observations in the near-infrared ;

It is derived in part by the Mars Express High Resolution Stereo Camera ( HRSC ) and the Rosetta Optical, Spectroscopic and Infrared Remote Imaging System ( OSIRIS ).

* Near Infrared Camera and Multi-Object Spectrometer

# REDIRECT Near Infrared Camera and Multi-Object Spectrometer

The Near Infrared Camera and Multi-Object Spectrometer ( NICMOS ) is a scientific instrument for infrared astronomy, installed on the Hubble Space Telescope ( HST ), operating from 1997 to 1999, and from 2002 to 2008.

hu: Near Infrared Camera and Multi-Object Spectrometer

* Near Infrared Camera and Multi-Object Spectrometer

* Near Infrared Camera and Multi-Object Spectrometer

It was replaced by the Near Infrared Camera and Multi-Object Spectrometer ( NICMOS ) in 1997.

* Near Infrared Camera and Multi-Object Spectrometer

* Near Infrared Camera and Multi-Object Spectrometer, a scientific instrument for infrared astronomy

While the WFPC2 took very deep optical images, nearby fields were simultaneously imaged by the Space Telescope Imaging Spectrograph ( STIS ) and the Near Infrared Camera and Multi-Object Spectrometer ( NICMOS ).

While the WFPC2 took very deep optical images, the fields were simultaneously imaged by the Space Telescope Imaging Spectrograph ( STIS ) and the Near Infrared Camera and Multi-Object Spectrometer ( NICMOS ).