The solar blind camera takes images of objects that
emit ultraviolet wavelengths.
Not exact matches
Some observations of how cosmic molecules
emit and absorb light at
ultraviolet wavelengths have hinted that the fine structure constant, responsible for the strength of electromagnetism, is not the same throughout the universe.
The problem with today's resist, however, is that it was originally developed for light sources that
emit so - called deep
ultraviolet light with
wavelengths of 248 and 193 nanometers.
The «colours» are due to differences in the surface temperature of starsw1: hotter stars
emit most of their light in the visible blue or
ultraviolet regions of the electromagnetic spectrum, whereas cooler stars radiate at longer
wavelengths, in the visible red or infrared regions (see Mignone & Barnes, 2011a).
When the star's
ultraviolet radiation strikes the gases in the nebula, they heat up, giving out radiation ranging in
wavelength from blue —
emitted by hot oxygen in the bubble near the star — to yellow —
emitted by hot hydrogen and nitrogen.
The distance to the quasar is so great (about 10 billion light - years) that the
emitted light is «stretched» by the expansion of the universe from an invisible
ultraviolet wavelength to a visible shade of violet by the time it reaches the 10 - meter Keck I telescope and the LRIS (Low Resolution Imaging Spectrometer) used for this discovery.
Although only 1 percent of the sun's energy is
emitted at
ultraviolet wavelengths between 200 and 300 nanometers, the decrease in this radiation from 1 July 1981 to 30 June 1985 accounted for 19 percent of the decrease in the total irradiance over the same period.»