Donald Scott: Electric Solar Wind | EU2016

https://www.youtube.com/watch?v=sFGb7NlUvgg

Published on 11 Oct 2016

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.

Dr. Donald Scott earned his Bachelors and Masters degrees in Electrical Engineering at the University of Connecticut. He earned a Doctorate in Electrical Engineering at the Worcester Polytechnic Institute, Worcester, Massachusetts, and was a member of the faculty of the Department of Electrical & Computer Engineering at the University of Massachusetts at Amherst from 1959 until his retirement in 1998. During that time, he was the recipient of several good-teaching awards and authored numerous scientific papers and chapters. In 1987, the McGraw-Hill Book Company published his 730-page textbook, An Introduction To Circuit Analysis – A Systems Approach. In addition, Dr. Scott published the classic, Electric Sky (2006), 256 pages of compelling material on the Electric Universe and plasma cosmology.
electric-cosmos.org