I don't get it..by definition you will always have a boundary layer in laminar flow-thats why you get a parabolic flow profile? you may get boundary layer mixing in turbulent flow-but you surely you don't want turbulent flow, thats why you want to replace natural convection with laminar flow through some sort of forced convection
if the question is how to create laminar flow in a telescope tube..thats a different question-the gun planetary imagers have some systems in place, I don't really know
but perhaps the best way to reduce natural convection probably is to cool the mirror with temperature sensing and feedback
take all the above with a pinch of salt I have never done any planetary imaging and own a GSO dob with not even a cooling fan so what would I know