Dependence of the Characteristics of Solar Wind Discontinuities and Shocks with Heliolatitude and Radial Distance
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/s11207-008-9244-2.pdf
Reference27 articles.
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2. Gopalswamy, N.A., Lara, R.P., Lepping, M.L., Kaiser, D., Berdichevsky, S., St. Cyr, O.C.: 2000, Interplanetary accleration of coronal mass ejection. Geophys. Res. Lett. 27, 145 – 148.
3. Gosling, J.T., Forsyth, R.J.: 2001, CME-Driven solar wind disturbances at high heliographic laritudes. Space Sci. Rev. 97, 87 – 98.
4. Gosling, J.T., Riley, P.: 1996, The acceleration of slow coronal mass ejection in the high speed wind. Geophys. Res. Lett. 23, 2867 – 2870.
5. Gosling, J.T., McComas, D.J., Phillips, J.L., Pizzo, V.J., Goldstein, B.E., Forsyth, R.J., Lepping, R.P.: 1995, A CME-driven solar wind disturbances observed at both low and high latitudes. Geophys. Res. Lett. 22, 1753 – 1756.
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