Traveling into the Colossal Dynanomic Slipstream Dimension will yield a great many surprises as SPACE1 has never done this before.
The best we can do at this time is to develop and run a simulation of a Jovian Ganymedian human landing to peer into the visibility keyhole of the Dynanomic Dimension.
At left is the keyhole camera view designed to minimize radiation and spectral effects.
We have developed a SIM potential view of what might be returned from a Jovian Ganymede moon mission using a kind of processed Dynanomic Vision inside the realm of this dimension.
PROCESS
The view is passed through light time in Jovian Ganymedian space. The first view is a limited keyhole view and other views that follow estimate images within Jupiter's great magnetic fields. Ganymede also has a metal core and creates magnetic lines of force that will affect the dimensional imagery obtained from the Dynanomic processes.
More tests are needed beyond the sim programming. In the final SIM view we see a glitch caused by a gravity radiation streak from the planet Jupiter. Corrections for radiation spikes and pulsations of a gravity field are an unknown process at this time.
The best SIM result is the keyhole technique, however we are also looking at a more involved global body imaging technique across the entire moon that can hone in a particular segment of Ganymedian detail at the landing site. Returning high resolution imagery will be the most challenging in this very remote cold environment.
Returning high resolution imagery will be the most challenging in this very remote cold environment. Probably the Jovian Ganymedian system is the smallest most remote system that can be handled at this time, without developing a variety of new techniques.
