Interpretation of the coronal magnetic field configuration of the Sun
- ISSN号:1674-4527
- 期刊名称:Research in Astronomy and Astrophysics
- 时间:2012.12
- 页码:1693-1700
- 分类:TM153[电气工程—电工理论与新技术] P182.7[天文地球—天文学]
- 作者机构:[1]Shandong Provincial Key Laboratory of Optical Astronomy & Solar-Terrestrial Environment, School of Space Science and Physics, Shandong University at Weihai, Weihai 264209, China, [2]State Key Laboratory of Space Weather, Chinese Academy of Sciences, Beijing 100190, China, [3]Institute of Mathematics & Physics, Aberystwyth University, Aberystwyth SY23 3BZ, UK
- 相关基金:supported by the National Natural Science Foundation of China(Grant Nos.40904047and 41174154); the Ministry of Education of China(20110131110058 and NCET-11-0305); by the Specialized Research Fund for State Key Laboratories
- 相关项目:湍动Alfven波与开场区日冕加热和太阳风加速
中文摘要:
bbl @ sdu. edu. cn