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Old 06-18-2009   #12 (permalink)
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Re: The Dominium Model: Part 2

Hi Eric,

Welcome. You bring up and excellent point/observation. Let us focus on the data actual observation (and not the theory that someone else surmised.) Yes, someone else did have a crack at explaining the evidence, but as you note, their explanation falls short. It is the physical evidence that is most important.

BTW, congratulations for figuring out the next moves, and that is that the escaping MPP’s are the drivers of the solar wind. You’re getting ahead of me, but I have never been one to avoid a direct question. Since you have preempted that move, let me summarize an overview of how that will happen:

MPP eventually escape the Sun’s surface (causing CME’s and twisted magnetic fields as they go. Some matter is pushed along in front of MPP. Continual nudging gives enough energy to also escape the Sun’s surface.

Now, we know (I believe confirmed by SoHo also) that the matter measured in the solar wind jumps from planet to planet of the equatorial ring of inner and outer planets. Within the ring of planets would also be away from where the MPP would want to travel. With fewer MPP drivers, the matter of the solar wind would not be accelerated as much as to more scarce matter remnant of the solar wind directly away from the poles.

The long and the short of your final question is "Yes, this observation does allign with a notion of gravitational repulsion."

In two moves your question will be given much more filling than I did just a moment ago. Please stay tuned. Also, tell as many people as you can about the ongoing, potentially pivotal, debate on this thread. There is more at stake than meets the eye.


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