Anyone who has imaged with a SCT has probably experienced "Mirror Flop" when near the meridian, and possibly at other orientations. This is caused in part by the basic design of the mirror mount itself. In order for the SCT to be focused, the primary mirror must move closer or further from the secondary mirror by sliding on a baffle tube that directs the light to the back of the scope. The mirror is moved and held in place by only one connection, which is the focuser. This single support point can not keep the weight of the mirror from shifting as it moves across the sky. The tolerances between the mirror holder and the baffle tube are not small enough to prevent this "flop" or shift. My first attempt to halt mirror movement was done with long bolts to connect to the mirror cell holder as seen here: Mirror Locks. These worked somewhat, but I still got some movement when guiding, and adjustment to maintain collimation was very difficult. So, I made the decision to install the Software Bisque Locking Collar. The following is a brief pictorial of the process.