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Interplanetary acceleration of coronal mass ejections
Abstract
Using an observed relation between speeds of CMEs near the Sun and in the solar wind, we determine an “effective” acceleration acting on the CMEs. We found a linear relation between this effective acceleration and the initial speed of the CMEs. The acceleration is similar to that of the slow solar wind in magnitude. The average solar wind speed naturally divides CMEs into fast and slow ones. Based on the relation between the acceleration and initial speed, we derive an empirical model to predict the arrival of CMEs at 1 AU.
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Citations
Cited by
Richardson, I. G., & Cane, H. V. (2010) · Solar Physics · doi:10.1007/s11207-010-9568-6 · Cited by 915
Observations of an extreme storm in interplanetary space caused by successive coronal mass ejections
Liu, Y. D., Luhmann, J. G., Kajdič, P., Kilpua, E. K. J., Lugaz, N., Nitta, N. V., Möstl, C., Lavraud, B., Bale, S. D., Farrugia, C. J., et al. (2014) · Nature Communications · doi:10.1038/ncomms4481 · Cited by 293
The Heliospheric Magnetic Field
Owens, M. J., & Forsyth, R. J. (2013) · Living Reviews in Solar Physics · doi:10.12942/lrsp-2013-5 · Cited by 263
Coronal mass ejections, interplanetary ejecta and geomagnetic storms
Cane, H. V., Richardson, I. G., & St. Cyr, O. C. (2000) · Geophysical Research Letters · doi:10.1029/2000gl000111 · Cited by 212
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Metadata
- Authors
- Gopalswamy, N., Lara, A., Lepping, R. P., Kaiser, M. L., Berdichevsky, D., & St. Cyr, O. C.
- Venue
- Geophysical Research Letters
- Publisher
- American Geophysical Union (AGU)
- Published
- 2000-01-15
- Volume
- 27
- Issue
- 2
- Pages
- 145-148
- ISSN
- 0094-8276 (ISSN-L)
- 1944-8007
- OpenAlex
- W1968256717
- Cited by
- 526
- References
- 0
- FWCI
- 14.08
- Type
- journal article
- Language
- en
- Open access
- closed
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- Gopalswamy, N., Lara, A., Lepping, R. P., Kaiser, M. L., Berdichevsky, D., & St. Cyr, O. C. (2000). Interplanetary acceleration of coronal mass ejections. Geophysical Research Letters. https://doi.org/10.1029/1999gl003639
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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.