These tables are necessary for the analysis of synthesis probability of kernels and the occurrence of these kernels, in the structure of «the solar wind». In the given tables, in columns 2, 3, 4, 5 presented the data of kernels «a» and «b» participating in synthesis. In columns 6, 7, 8 given the kernels «C», received during the process of synthesis of kernels «a» and «b». In columns 9, 10, 11 presented the results of calculations of power and high-speed characteristics of a kernel «C», calculated by the formulas:

                          Δm=ΔD_a+ΔD_b—ΔD_c,         keV                                                            (4.1)

                          v_c=(Δm/M_c) ^. C,                km/s                                                          (4.2)

In formula (4.1), part of the weight and the energy allocated at moment of synthesis of kernel «C» is calculated. In formula (4.2) the high-speed characteristic of kernel «c» is defined.

Having divided Δm on weight of kernel «C», Mc, received at synthesis, we shall receive its high-speed parameter. From the third law of Newton it is emitted, that the speed of kernel «C» will depend on the attitude of weights:

                                   v_c~(Δm/M_c).

As,Δm ^. v_iz= M_c ^. v_c

Where v_iz=C — speed of radiation close to speed of light;                

M_c, v_c — weight and speed of kernel «C», received during the synthesis of kernels «A» and «B».

Hence,

                     v_c=(Δm/M_c) ^. C=(Δm/M_c) ^. v_iz

Speed and impulse of kernel «c», depends and proportional to the radiation impulse:

                       P_c= M_c ^. v_c ,

                       P_iz= Δm ^. v_iz ,

                       P_c ~ P_iz .

For the simplification of the analysis, we shall accept the assumption:

  — Impulses of kernels «A» and «B» participated in the synthesis, compensate each other, and their sum is equal to zero.

Let’s calculate and analyze the high-speed characteristics of kernels with z=1 – 30, a part of the solar wind, considering two variants of synthesis            

                                  Variant 1
The calculations presented in the table №T-4.2.
For the simplification of the analysis, the results of kernels high-speed characteristics are written in the form of table №T-4.2a and schedules №G-4.1, №G-4.1a, №G-4.1b are constructed. In this variant, the synthesis of kernels of «the solar wind» occurs by merge of kernels «a» and «b», having z=1 — 16 for both kernels.

                                          (69)  Table № T-4.2a 

                                                        (70)   Schedule №G-4.1

                                                  (71) Schedule №G-4.1a

                                                      (72)  Schedule №G-4.1b

                   Variant 2:
The calculations are presented in the table №T-4.3.
The high-speed characteristics of kernels, that are a part of «the solar wind», are written as table №T-4.3a and schedules №G-4.2, №G-4.2a, №G-4.2b are constructed.