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Analysis of the ICME on 24 August 2001

Published online by Cambridge University Press:  01 September 2008

Nedelia A. Popescu*
Affiliation:
Astronomical Institute of Romanian Academy, Bucharest, RO-040557, Romania email: nedelia@aira.astro.ro
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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.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2009

References

Lepri, S. T. & Zurbuchen, T. H. 2004, J. Geophys. Res., 105, 29, 231Google Scholar
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