NSSC OpenIR  > 空间科学部
太阳风扰动传输模式研究进展
Alternative TitleResearch Progresses in Modeling the Propagation of Solar Wind Disturbances
史良文; 申成龙; 汪毓明; 沈芳
Department空间科学部
Source Publication天文学进展
2013
Volume31Issue:3Pages:267-286
ISSN1000-8349
Language中文
Keyword太阳风 日冕物质抛射 行星际空间 空间天气
Abstract随着观测手段、理论模型和数值方法的发展,人们对各种太阳风扰动如日冕物质抛射,以及相关的空间天气效应的认识和理解越来越深入。为获取行星际背景磁场、背景太阳风参数和日冕物质抛射、激波等太阳风扰动的传播参数,人们建立发展了各种模式;在这些获取的参数基础上,建立了各种太阳风扰动的传播模式,从而为空间天气预报提供了必要的经验和理论模型支持。根据这些模式所研究和描述物理量的不同,将这些参数获取模式和传播预报模式分为背景磁场获取模式、背景太阳风参数获取模式、日冕物质抛射传播参数获取模式、日冕物质抛射偏转模式、日冕物质抛射(激波)传播模式以及基于三维磁流体力学的数值模拟方法,并分别概述性地总结了各种模式的特点及其用途。
Other AbstractWith the development of observation technology, theoretical models and numerical sim-ulation methods, peoples understanding of solar wind disturbances, e.g., coronal mass ejections (CMEs), and their resultant space weather effects are continuously advanced. Various models have been developed to obtain the parameters of interplanetary magnetic field (IMF), solar wind plasma, CMEs, shocks, and other disturbances. These models have formed the necessary supports for space weather forecasting. According to the function and purpose, these models could be classified as background IMF obtaining models, background solar wind obtaining models, CME kinematic parameters obtaining models, CME deflection models, CME (shock) propagation models and numerical MagnetoHydro-Dynamic (MHD) simulation methods. In this paper, we give a brief review of these models. First, the background IMF models are introduced, such as the potential field source surface (PFSS) model and the current sheet-source surface (CSSS) model. Then, the Wang-Sheeley-Arge (WSA) model and the interplanetary scintillation (IPS) model, which could be used to get the back-ground solar wind parameters, are also reviewed. In addition, the models to get the CMEs prop-agation parameters are reviewed, for example: type II radio bursts model, various cone models, graduated cylindrical Shell (GCS) model and some triangulation models. It is important in space weather forecasting that if and when the solar wind disturbances will arrive at the Earth. In this paper, we show the coronal hole (CH) compression models, the magnetic energy density gradient models (MEDG) and the magnetic frozen-in models. These models could be used to forecast whether a CME would arrive at the Earth. In addition, we also introduce the shock time of arrival model (STOA), the interplanetary shock propagation model (ISPM), the Hakamada-Akasofu-Fry (HAF) model and the shock propagation model (SPM), which were developed to forecast solar wind disturbance arrival time. Finally, we give a brief review of MHD numerical simulation models about the propagation of the solar wind disturbance.
Indexed ByCSCD
Citation statistics
Document Type期刊论文
Identifierhttp://ir.nssc.ac.cn/handle/122/5063
Collection空间科学部
Recommended Citation
GB/T 7714
史良文,申成龙,汪毓明,等. 太阳风扰动传输模式研究进展[J]. 天文学进展,2013,31(3):267-286.
APA 史良文,申成龙,汪毓明,&沈芳.(2013).太阳风扰动传输模式研究进展.天文学进展,31(3),267-286.
MLA 史良文,et al."太阳风扰动传输模式研究进展".天文学进展 31.3(2013):267-286.
Files in This Item: Download All
File Name/Size DocType Version Access License
2013313267.pdf(1698KB) 开放获取CC BY-NC-SAView Download
Related Services
Recommend this item
Bookmark
Usage statistics
Export to Endnote
Google Scholar
Similar articles in Google Scholar
[史良文]'s Articles
[申成龙]'s Articles
[汪毓明]'s Articles
Baidu academic
Similar articles in Baidu academic
[史良文]'s Articles
[申成龙]'s Articles
[汪毓明]'s Articles
Bing Scholar
Similar articles in Bing Scholar
[史良文]'s Articles
[申成龙]'s Articles
[汪毓明]'s Articles
Terms of Use
No data!
Social Bookmark/Share
File name: 2013313267.pdf
Format: Adobe PDF
All comments (0)
No comment.
 

Items in the repository are protected by copyright, with all rights reserved, unless otherwise indicated.