Alice is
an ultraviolet imaging spectrometer whose purpose is to study the atmospheric structure and composition of Pluto.
When New Horizons arrives at the Pluto system, onboard science instruments such as Alice, a sensitive
ultraviolet imaging spectrometer, will reveal even more about the composition and structure of the dwarf planet's dynamic atmosphere.
As New Horizons glides behind Pluto and its shadow during the flyby,
an ultraviolet imaging spectrometer aboard the spacecraft, named Alice, will analyze the filtered sunlight that passes through Pluto's atmosphere.
During this period, in - flight tests were conducted on the spacecraft's Alice
ultraviolet imaging spectrometer and Pluto Energetic Particle Spectrometer Science Investigation (PEPSSI), as well as LORRI, and New Horizons passed the orbit of Mars in April 2006.
Images from Cassini's
ultraviolet imaging spectrometer (UVIS), obtained from an unusually close range of about six Saturn radii, provided a look at the changing patterns of faint emissions on scales of a few hundred miles (kilometers) and tied the changes in the auroras to the fluctuating wind of charged particles blowing off the sun and flowing past Saturn.
Not exact matches
Intense extreme
ultraviolet FEL pulses were directed at the clusters and the resultant energy distribution of electrons knocked out of the clusters was measured using a «velocity map
imaging spectrometer».
Wide Field Optical
Spectrometer (WFOS) The Wide Field Optical
Spectrometer (WFOS) will provide near -
ultraviolet and optical (0.3 — 1.0 μm wavelength)
imaging and spectroscopy over a more than 40 square arcminute field - of - view.
Images from the Extreme
ultraviolet Imaging Telescope (EIT) and the Coronal Diagnostics
Spectrometer (CDS) on SOHO show the hot gases of the ever - changing corona reacting to the evolving magnetic fields rooted in the solar surface.
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.
In addition to providing important information on its own, NGIMS would complement other instruments aboard, specifically the
Imaging Ultraviolet Spectrometer, which would also measure gas composition.