# REDIRECT Fourier transform infrared spectroscopy

# REDIRECT infrared

# REDIRECT Forward looking infrared

# ultraviolet, visible, infrared imaging spectrometer

# A bank of forward firing grenade launchers or dischargers mounted on either side of the turret, which can fire grenades dispensing an aerosol smoke screen opaque to infrared light.

# Two infrared lights, one on each side of the main gun, continuously emit coded pulsed-infrared jamming when an incoming ATGM has been detected.

# REDIRECT infrared divergence

# REDIRECT infrared homing

# REDIRECT infrared homing

# REDIRECT infrared homing

# REDIRECT infrared homing

# REDIRECT infrared homing

# REDIRECT infrared homing

# REDIRECT infrared homing

# REDIRECT infrared homing

# REDIRECT infrared homing

# REDIRECT infrared homing

# REDIRECT infrared homing

# REDIRECT infrared homing

# REDIRECT Forward looking infrared

# Scanning infrared radiometers

# Infrared light curtain — When pressed to the whiteboard surface, the finger or marker sees the infrared light.

# Laser light curtain — An infrared laser is located in each upper corner of the whiteboard.

# Hybrid Ultrasound and Infrared — When pressed to the whiteboard surface, the marker or stylus sends out both an ultrasonic sound and an infrared light.

# dust mass spectrometer

# neutral gas mass spectrometer

# A sample is loaded onto the mass spectrometer, and undergoes vaporization

# A micrometeorite momentum spectrometer ( or micrometeorite detector ) that consisted of two diaphragm and microphone combinations.

The despun section's instruments included the camera system ; the near infrared mapping spectrometer to make multi-spectral images for atmospheric and moon surface chemical analysis ; the ultraviolet spectrometer to study gases ; and the photo-polarimeter radiometer to measure radiant and reflected energy.

As reported by Richard Kerr, " A spectrometer ( the Moon Mineralogy Mapper, aka " M3 "), detected an infrared absorption at a wavelength of 3. 0 micrometers that only water or hydroxyl – a hydrogen and an oxygen bound together – could have created.

A common laboratory instrument that uses this technique is a Fourier transform infrared ( FTIR ) spectrometer.

* Sensors: wide-and narrow-angle cameras with digital tape recorder, infrared spectrometer and radiometer, ultraviolet spectrometer, radio occultation and celestial mechanics.

* Sensors: wide-and narrow-angle cameras with digital tape recorder, infrared spectrometer and radiometer, ultraviolet spectrometer, radio occultation and celestial mechanics

* Sensors: twin narrow-angle cameras with digital tape recorder, ultraviolet spectrometer, infrared radiometer, solar plasma, charged particles, magnetic fields, radio occultation and celestial mechanics

A scan platform was mounted on the bottom of the frame, on which were attached the mutually bore-sighted science instruments ( wide-and narrow-angle TV cameras, infrared radiometer, ultraviolet spectrometer, and infrared interferometer spectrometer ).

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.

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 ).

Scientific instruments included a gamma-ray spectrometer for energies between 0. 3 — 3 MeV ( 50 – 500 pJ ), a triaxial magnetometer, a meteorite detector, instruments for solar-plasma studies, and devices for measuring infrared emissions from the Moon and radiation conditions of the lunar environment.

The craft was powered by twin large solar panels and instruments included an antenna dish, cameras, spectrometer, infrared sounder, magnetometers ( MISCHA ), and plasma probes.

The images also showed the nucleus to be dark, and the infrared spectrometer readings measured a nucleus temperature of 300 K to 400 K, much warmer than expected for an ice body.

The craft was powered by twin large solar panels and instruments included an antenna dish, cameras, spectrometer, infrared sounder, magnetometers ( MISCHA ), and plasma probes.

The craft was powered by twin large solar panels and instruments included an antenna dish, cameras, spectrometer, infrared sounder, magnetometers ( MISCHA ), and plasma probes.

The Phobos 2 infrared spectrometer ( ISM ) obtained 45000 spectra in the near infrared ( from 0. 75 to 3. 2 µm ) in the equatorial areas of Mars, with a spatial resolution ranging from 7 to 25 km, and 400 spectra of Phobos at 700 m resolution.