Hostname: page-component-8448b6f56d-gtxcr Total loading time: 0 Render date: 2024-04-18T15:00:14.574Z Has data issue: false hasContentIssue false

3D reconstruction of solar magnetoacoustic waves

Published online by Cambridge University Press:  01 November 2008

Adrian Sabin Popescu*
Affiliation:
Astronomical Institute of the Romanian Academy, Str. Cutitul de Argint 5, RO-040557 Bucharest, Romania email: sabinp@aira.astro.ro
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Using a new multi-wavelength technique applied on the solar corona SOHO/EIT images containing magnetoacoustic waves (EIT waves), we constrain the wave phase velocity and, as well, some β-model, height related considerations for the vertical extent of the wave, applied on the particular EIT wave triggered by the eruptive event from 15th of August, 2001.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2009

References

Athay, R. G., White, O. R., Lites, B. W., & Bruner, E. C. 1980, SP 66, 357Google Scholar
Delaboudinière, J.-P., Artzner, G. E., Brunaud, J., et al. 1995, SP 162, 291Google Scholar
Gary, G. A. 2001, SP 203, 71Google Scholar
Priest, E. R. 1987, in: McCormac, B. M. (ed.), Solar Magneto-hydrodynamics, Geophys. and Astrophys. Mon. 21, D. Reidel Publishing Company, Dordrecht, Holland, p. 189Google Scholar
Malherbe, J. H. & Priest, E. R. 1983, A&A 123, 80Google Scholar
Popescu, A. S. & Mierla, M. 2008, in: Mioc, V., Dumitrache, C., Popescu, N. A. (eds.), Exploring the Solar System and the Universe, AIP Conference Proceedings Series, Vol. 1043, p. 309.Google Scholar