The stream of particles radiating from the Sun is called the ‘Solar Wind’. It is observed to exhibit two different forms: the fast solar wind and the slow solar wind. In this talk, Dr. Donald Scott presents his new interpretation of the reasons why the densities and velocities of these two different ‘winds’ exist. Making use of Juergen’s Electric Sun model, he offers a clear understanding of how and why the different locations on the Sun’s surface from which each of these streams originate causes their differing properties. An electric mechanism, consistent with the ES model, is shown to be easily capable of providing the observed acceleration.
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