Analysis of Radial Dependences of the Electron Concentration and Plasma Velocity in the Region of Accelerated Solar Wind
- 作者: Yakovlev O.I.1, Yakovlev Y.O.1
-
隶属关系:
- Kotelnikov Institute of Radioengineering and Electronics, Fryazino Branch, Russian Academy of Science
- 期: 卷 57, 编号 4 (2019)
- 页面: 237-242
- 栏目: Article
- URL: https://journals.rcsi.science/0010-9525/article/view/153365
- DOI: https://doi.org/10.1134/S0010952519040087
- ID: 153365
如何引用文章
详细
Results of experimental studies of the electron concentration and near-solar plasma velocity dependences on the heliocentric distance obtained in 1970–2012 by the method of radio transillumination by signals of spacecraft for the region of 3–50 solar radii are presented. A comparative analysis of different approximations of these dependences is given and it is shown that joint analysis of the data on the plasma velocity and concentration with allowance for independence of the plasma integral flux on the heliocentric distance makes it possible to find analytical expressions corresponding well to experimental data. Analytical approximations and graphs of dependences of the velocity, concentration, acceleration, force, and kinetic energy on the distance in the regions of solar wind acceleration for low and moderate solar activity are presented.
作者简介
O. Yakovlev
Kotelnikov Institute of Radioengineering and Electronics, Fryazino Branch, Russian Academy of Science
编辑信件的主要联系方式.
Email: oiy117@ire216.msk.su
俄罗斯联邦, Fryazino
Yu. Yakovlev
Kotelnikov Institute of Radioengineering and Electronics, Fryazino Branch, Russian Academy of Science
Email: oiy117@ire216.msk.su
俄罗斯联邦, Fryazino
补充文件
