Physics of the Sun and stars
Copyright © 2010 by Stanislav Kozlov
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4.2. Modern theories about «a solar wind» and about a star structure
One of the most interesting natural phenomena – is the «a solar wind» (or a star wind). Modern researchers lead huge work on gathering the information about it. But unfortunately, the base theories about the Sun structure, written almost hundred years ago, like other theories in modern astrophysics, have become outdated, and the collected information remains without application. Actually, as the analysis of blood of the human gives the information on its health, the analysis of parameters of «a solar wind» can give us huge information about a structure and about its state.
Why until now there is no such analysis?
First, it is necessary to collect a huge quantity of information.
Second, a group of analysts into which should include experts on the nuclear physics, physicist of plasma, thermo physics and some other is necessary.
Third, the theory about star and the Sun structure has become outdated and mismatches the validity, means, it is erroneous. Hence, the analysis of all the data collected, based on the erroneous theory, will be erroneous.
Fourth, because of the existing mistake in the theory about the Sun structure, researchers do cannot understand the value of data available to them about a star and «a solar wind», and the actual information this data carries.
Let’s try to correct almost hundred years old mistake in the theory of the Sun structure.
Sun structure
According to still considered as modern theory, the Sun is consisted of a kernel where under the weight of the top layers there is a thermonuclear synthesis of kernels of hydrogen in kernels of helium.
At the process of thermonuclear synthesis, in a kernel of the Sun, energy is allocated. This energy, having passed radiant and convection zones, is transferred into an atmosphere. In the top layers of an atmosphere of a star, under the action of variable magnetic field, particle, kernel of atoms, ions and electrons are being thrown out in a space. The speed of the thrown out particles is high and different.
