Ultraviolet data collected by NASA's MAVEN spacecraft was used to construct these images
showing ultraviolet emissions before (left) and during (right) the storm
This image of the Mars night side
shows ultraviolet emission from nitric oxide (abbreviated NO).
Figure 1 (a) represents the corrected visible light from Neptune from 1950 to 2006; (b) shows the temperature anomalies of the Earth; (c) shows the total solar irradiance as a percent variation by year; (d)
shows the ultraviolet emission from the Sun (Source: Hammel and Lockwood (2007)-RRB-.
Not exact matches
Recently, signatures of CO Cameron and CO2 + doublet
ultraviolet auroral
emissions have been detected with SPICAM (Gérard et al. 2015); they
showed that the Mars aurora is a temporary and spatially localized phenomenon appearing near the open - closed magnetic field line boundary in cusp - like structures.
These star - formation rate estimators include the
ultraviolet light that is emitted from young stars, the infrared light that
shows how much of the
ultraviolet light was absorbed by dust, and the nebular
emission lines that are caused by young stars making the clouds of gas around them glow and radiate.