Physics of the Sun and stars
Copyright © 2010 by Stanislav Kozlov
All rights reserved. No part of this book may be reproduced in any form or by any
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4.5. «A solar wind»
We have considered how the Sun is arranged, using the new theory developed by us, based on the laws of classical physics. If we lean on the theory given, we see that the information on a solar wind gives us an invaluable knowledge of the star and gives another, absolutely more powerful value. For the analysis of the solar wind it is necessary to define the sources and the nature of its formation.
– Sources of «a solar wind»
Sources of a solar wind are:
– «The active zone» – a zone where the thermonuclear synthesis leads to allocation of most of the energy, is the top part of the atmosphere: the photosphere, the chromosphere, and the bottom part of the crown;
– «Dark spots» – place of break of the gas-plasma mix on a surface of the Sun, through «the active zone». It’s probably possible to add coronary holes to this list, but their deeper studying is necessary for this purpose.
– The nature of formation of «a solar wind»
– In the active zone there are thermonuclear reactions of synthesis in which, kernels and particles receive an impulse during the moment of energy allocation and are a part of the solar wind.
– In «the dark spot» – throttling of the gas-plasma mix occurs (fig. №R-4.12), and the emission of gas-plasma mix, during the nuclear explosions inside the stars (fig. №R-4.13). Particles, atoms and kernels receive high speed due to the expiration in space of gas and plasma, through the hole in the active zone. Since in the nutria of a star, the gas-plasma mix has high values of temperature and pressure, in this case it is possible to hit in the structure «solar wind» of kernels that are heavier than Zn and of kernels in which the synthesis occurs, without the energy allocation, or with minimum allocation.
