Characteristics of coronal mass ejections associated with interplanetary shocks
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/BF00679079.pdf
Reference4 articles.
1. Gosling, J. T.: 1993,J. Geophys. Res. 98, 18 937.
2. Gosling, J. T., Hildner, E., MacQueen, R. M., Munro, R. H., Poland, A. I., and Ross, C. L.: 1976,Solar Phys. 48, 389.
3. Howard, R. A., Sheeley, N. R., Jr., Koomen, M. J., and Michels, D. J.: 1985,J. Geophys. Res. 90, 8173.
4. Sheeley, N. R., Jr., Howard, R. A., Kommen, M. J., Michels, D. J., Schwenn, R., Mühlhäuser, K. H., and Rosenbauer, H.: 1985,J. Geophys. Res. 90, 163.
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1. On observing mass ejections in the interplanetary medium;Solar Physics;1999
2. Disconnection of coronal field lines due to the emergence of new photospheric flux as the cause of CMEs and interplanetary shocks;Astrophysics and Space Science;1996
3. A possible scenario for the associated occurrence of flares, prominence eruptions, coronal mass ejections, and coronal holes in relation to interplanetary shocks;Advances in Space Research;1996-01
4. Disconnection of Coronal Field Lines Due to the Emergence of New Photo-Spheric Flux as the Cause of CMES & Interplanetary Shocks;International Astronomical Union Colloquium;1996
5. A solar scenario for the associated occurrence of flares, eruptive prominences, coronal mass ejections, coronal holes, and interplanetary shocks;Solar Physics;1995-10
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