Not exact matches
Imaging the cosmos at near -
infrared wavelengths
allowed the astronomers to see objects that are both obscured by dust, and extremely distant [2], created when the Universe was just an infant.
Infrared Multi-object Spectrometer (IRMS) The Infrared Multi-object Spectrometer (IRMS) will allow close to diffraction - limited imaging and slit spectroscopy over a 2 arcminute diameter field - of - view at near - infrared wavelengths (0.8 —
Infrared Multi-object Spectrometer (IRMS) The
Infrared Multi-object Spectrometer (IRMS) will allow close to diffraction - limited imaging and slit spectroscopy over a 2 arcminute diameter field - of - view at near - infrared wavelengths (0.8 —
Infrared Multi-object Spectrometer (IRMS) will
allow close to diffraction - limited
imaging and slit spectroscopy over a 2 arcminute diameter field - of - view at near -
infrared wavelengths (0.8 —
infrared wavelengths (0.8 — 2.5 μm).
The photodetector array camera and spectrometer (PACS) aboard the Herschel Space Observatory
allows imaging observations in the far
infrared at unprecedented resolution, i.e. at better than 6» to 12» over the wavelength range of 60 -LCB- \ mu -RCB- m to 210 -LCB- \ mu -RCB- m. Together with the results from ground - based observations, these spatially resolved data can be modelled to determine the nature of the debris and its evolution more reliably than would be possible from unresolved data alone.
Thermal
imaging allows heat levels to be detected by measuring
infrared radiation, producing images of that radiation called thermograms.
Infrared Thermal
Imaging is an advanced, non-destructive technology that
allows us to show you things about your home that no one can show you with conventional inspection methods.