Diagnostics of solar wind streams

Q4 Physics and Astronomy

Astronomical and Astrophysical Transactions Pub Date : 2007-12-13 DOI:10.1080/10556790701610449

N. Lotova, K. Vladimirskii, V. Obridko

引用次数: 1

Abstract

Up-to-date methods of investigation of solar wind generation are applied to study the types of the streams that form the inhomogeneous jet structure of circumsolar plasma. The particularities of this structure are analysed at the maximum and transition to the declining phase of cycle 23.

查看原文本刊更多论文

太阳风的诊断

应用最新的研究太阳风产生的方法来研究形成太阳周围等离子体不均匀射流结构的流的类型。分析了该构造在第23旋回最大期和向衰退期过渡时的特殊性。

本文章由计算机程序翻译，如有差异，请以英文原文为准。

求助全文

约1分钟内获得全文求助全文

来源期刊

Astronomical and Astrophysical Transactions Physics and Astronomy-Instrumentation

CiteScore

0.40

自引率

0.00%

发文量

期刊介绍： Astronomical and Astrophysical Transactions (AApTr) journal is being published jointly by the Euro-Asian Astronomical Society and Cambridge Scientific Publishers, The journal provides a forum for the rapid publication of material from all modern and classical fields of astronomy and astrophysics, as well as material concerned with astronomical instrumentation and related fundamental sciences. It includes both theoretical and experimental original research papers, short communications, review papers and conference reports.