Sharp Changes of Solar Wind Ion Flux and Density Within and Outside Current Sheets
Author:
Publisher
Springer Science and Business Media LLC
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://link.springer.com/content/pdf/10.1007/s11207-011-9719-4.pdf
Reference47 articles.
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2. Borodkova, N.L., Zastenker, G.N., Riazantseva, O., Richardson, J.D.: 2005, Large and sharp solar wind dynamic pressure variations as a source of geomagnetic field disturbances in the outer magnetosphere (at the geosynchronous orbits). Planet. Space Sci. 53, 25 – 32.
3. Borovsky, J.E.: 2008, Flux tube texture of the solar wind: Strands of the magnetic carpet at 1 AU. J. Geophys. Res. 113, A08110.
4. Borrini, G., Gosling, J., Bame, S., Feldman, W., Wilcox, J.: 1981, Solar wind helium and hydrogen structure near the heliospheric current sheet: A signal of coronal streamers at 1 AU. J. Geophys. Res. 86, 4565 – 4573.
5. Briggs, P.R., Armstrong, T.P.: 1984, Observations of interplanetary energetic ion enhancements near magnetic sector boundaries. Geophys. Res. Lett. 11, 27 – 30.
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