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Analysis of the ICME on 24 August 2001
Published online by Cambridge University Press: 01 September 2008
Abstract
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The analysis of in-situ data recorded by Ulysses for the ICME on 24 August 2001 is carried out, using different signatures such as He++ abundance enhancement, low ion temperature, low velocity, and anomalies of abundance and charge state of heavy ion species.
Keywords
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 4 , Symposium S257: Universal Heliophysical Processes , September 2008 , pp. 295 - 297
- Copyright
- Copyright © International Astronomical Union 2009
References
Neugebauer, M. & Goldstein, R. 1997, in: Crooker, N. et al. (eds.), Coronal Mass Ejections, AGU, p. 245Google Scholar
Oncica, A., Popescu, N., & Dumitrache, C. 2008, in: Mioc, V. et al. (eds), Exploring the Solar System and the Universe, AIP Conference Proceedings, 1043, 323Google Scholar
Richardson, I. G., Farrugia, C. J., & Cane, H. V. 1997, J. Geophys. Res., 102, 4691CrossRefGoogle Scholar
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