10
For all configuration files you must ensure that the Tamarisk is also set to the complementary imaging
mode (8bit, 14bit, or SuperFrame). This can be accomplished in the DRS Camera Control Software or
with the SOTI GUI.
Image seen in eBUS Player
Use when Pre-AGC raw 14-bit data is
needed. This can be used to create
usable video when histogram scaling is
applied.
Live display will show low
contrast greyscale video with
no AGC applied, no symbology.
Use when Post AGC numeric data is
needed. This can be used to create
usable video when histogram scaling is
applied. (No pixel temperature data
will be available on GT models)
eBus Player live image should
be good contrast greyscale
video with AGC applied.
Viento-G cameras – Use when Pre-
AGC raw 14-bit data is needed. This
data is the same data as is provided by
the 14-bit Mono Through mode.
Viento-GT cameras – Use when 16-bit
temperature calibrated data values for
every pixel is needed
Live display initially shows
almost flat image, very little
contrast, this will improve once
the histogram scaling is auto-
configured.
SuperFrame Color
(YUV422 video)
Use when YUV422 video that includes
AGC, Image Overlays, and Color
Palettes is needed. No calibrated pixel
temperature data will be available.
Live display will show a high
contrast image with AGC, color
palette and image overlays
applied.
Viento GT cameras will also
show temperature scale and
region of interest with
temperature.