The color image of the glory (top) is a composite of these three photos, which were
taken at different wavelengths of light during the phenomenon.
Not exact matches
The team made observations
at many
different wavelengths, optimised for
different features and cloud layers in Jupiter's atmosphere, to create the first global spectral maps of Jupiter
taken from Earth.
By looking
at high - resolution images
taken by SDO and STEREO over the same time period and in
different wavelengths, Alzate and her colleagues
at the University of Aberystwyth were able to focus down on the cause of the puffs and the interaction between the small and large - scale eruptions.
This colour picture was created from images
taken through four
different filters
at near - infrared
wavelengths.
Io imaged in
different infrared
wavelengths — the eruptions were observed
taking place
at the Rarog and Heno calderas, and later
at 201308C as exhibited in d (Image: Katherine de Kleer / UC Berkeley / Gemini Observatory)