SMALL-SCALE STRUCTURES IN THE SOLAR CORONA

被引：0

作者：

HARBAL, SR

机构：

来源：

SPACE SCIENCE REVIEWS | 1994年 / 70卷 / 1-2期

关键词：

SOLAR CORONA; SOLAR WIND; SMALL SCALE STRUCTURES;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The observational characteristics of the small scale magnetic structures are summarized. The temperature structure and temporal variability of the emission from coronal bright points, that pervade the source region of the solar wind in coronal holes and the quiet sun, and from active regions are shown to be remarkably similar. Particular emphasis is given to observations, potentially feasible with SOHO, that could resolve some of the outstanding issues regarding the role of the small scale magnetic structures in the energy balance and properties of the solar wind.

引用

页码：37 / 46

页数：10

共 18 条

[1]

ARNDT MB, 1994, IN PRESS SOLAR PHYS

[2] DYNAMICAL PROPERTIES OF THE SOLAR CORONA FROM INTENSITIES AND LINE WIDTHS OF EUV FORBIDDEN LINES OF SI-VIII, FE-XI, AND FE-XII [J].