IDAS planetary imaging filters are specialized filters designed with tuned passbands
intended to enhance features of specific planetary targets. Note that these filter bandpasses are at (or beyond) the edges of the visual spectrum. The camera and optical imaging components must be designed for proper operation at these wavelengths.
UV372-80
This filter is used for imaging vapor and clouds on Mars and Venus as
well as for imaging biological subjects. The UV bandpass design enhances in-band contrast by
aggressively eliminating out-of-band light:
Leakage of Visible Band: <1/1,000,000
Leakage from 680nm to 1,000nm: <1/150,000
Leakage from 1,000 to 1,200nm: <1/3,000
Available in 31.7mm(M28.6) and 52mm sizes
VW-1 This filter is used for imaging Venus (increases contrast for lower atmosphere cloud structures).
BE410 This filter is used to image Mars. It enhances the visibility of atmospheric water vapor clouds.
BPF This filter is used to image Jupiter and Saturn. The bandpass enhances contrast in the methane band.
IDAS planetary imaging filters are specialized filters designed with tuned passbands
intended to enhance features of specific planetary targets. Note that these filter bandpasses are at (or beyond) the edges of the visual spectrum. The camera and optical imaging components must be designed for proper operation at these wavelengths. 
