A new four-plasma categorization scheme for the solar wind-Reference-Cited by-同舟云学术

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A new four-plasma categorization scheme for the solar wind

Published:2015-01 Issue:1 Volume:120 Page:70-100
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Xu Fei¹²,Borovsky Joseph E.³⁴⁵

Affiliation:

1. Physics Department; Nanjing University of Information Science and Technology; Nanjing China

2. CSPAR; University of Alabama; Huntsville Alabama USA

3. Center for Space Plasma Physics; Space Science Institute; Boulder Colorado USA

4. AOSS; University of Michigan; Ann Arbor Michigan USA

5. Physics Department; Lancaster University; Lancaster UK

Funder

Lancaster University by Science and Technology Funding Council

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

http://onlinelibrary.wiley.com/wol1/doi/10.1002/2014JA020412/fullpdf

Reference150 articles.

1. The Fe/O elemental abundance ratio in the solar wind;Aellig;J. Geophys. Res.,1999a

2. The Fe/O elemental abundance ratio in the solar wind;Aellig;AIP Conf. Proc.,1999b

3. A model for the sources of the slow solar wind;Antiochos;Astrophys. J.,2011

4. Slow wind and magnetic topology in the solar minimum corona in 1996-1997;Antonucci;Astron. Astrophys.,2005

5. Improved method for specifying solar wind speed near the Sun;Arge;AIP Conf. Proc.,2003

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