Thank-you, Chip, for your question.  I really appreciate your interest and concern.  I want you to know how much this means to me. I also want you to know that I have the same concern, but I very much believe it is possible to overcome our consternation regarding these obstructing variables with hard work and well-founded intentions.

 

More specifically, I have tried a number of different algorithms, including a distributed simulation where a very large number of particles are simulated in a distributed manner, recognizing it would be very difficult and would take significantly longer to do this in an undistributed fashion.  As promising as this may sound, unfortunately the back flow was different than what was expected.  As I am sure you can imagine, the color change was shocking, not to mention the odor.  Plus it was also pretty sticky.

 

That being said, the overall strategy was adjusted in both time and space, allowing for changes in the precession axis, although admittedly small, with the belief, however, that small adjustments would magnify over the distance required to realize the difference between the heliosheath and the heliopause.

 

As you rethink this, take also into consideration the time constant, particularly as would be the case described in the early work of Niels Bohr.  With that in mind, the offensive odor is no longer problematic, as is depicted in the following:

                                                    

​​

​​

​

​

I probably should leave it at that.  Obviously, there is room for interpretation, especially in deference to the various situations posed by the multiverse.  I will just say, however, that the crispy edges and lightly browned under-surface make all the work worthwhile.

 

If you have any other questions or if any other readers have different perspectives, please feel free to share your ideas.  You can post your comments on the website.