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On the dynamics of eruptive prominences

Published online by Cambridge University Press:  06 January 2014

Laura A. Balmaceda ,
Hebe Cremades ,
Guillermo Stenborg ,
Carlos Francile ,
Leonardo Di Lorenzo  and
Fernando López
Laura A. Balmaceda
Affiliation:
ICATE/CONICET-UNSJ, CC 49, 5400 San Juan, Argentina email: lbalmaceda@icate-conicet.gob.ar Instituto Nacional de Pesquisas Espaciais, São José dos Campos, Brazil
Hebe Cremades
Affiliation:
UTN - Facultad Regional Mendoza and CONICET, Mendoza, Argentina
Guillermo Stenborg
Affiliation:
George Mason University, Fairfax, VA 22030, USA
Carlos Francile
Affiliation:
OAFA - Universidad Nacional de San Juan, San Juan, Argentina
Leonardo Di Lorenzo
Affiliation:
Universidad Nacional de San Luis, San Luis, Argentina
Fernando López
Affiliation:
ICATE/CONICET-UNSJ, CC 49, 5400 San Juan, Argentina email: lbalmaceda@icate-conicet.gob.ar
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Abstract

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To contribute to the understanding of the physical mechanisms at work during the initial phase and early evolution of erupting prominences, we analyze combined observations from ground-based and space-borne instruments. We present two case studies, which occurred at two different phases of the solar cycle, namely on March 2, 2002 and on April 16, 2012. In particular, we show the results of a morphological and kinematical analysis and interpret them in terms of available theoretical models.

Keywords

Prominence dynamicsprominence eruption
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S300: Nature of Prominences and their role in Space Weather , June 2013 , pp. 179 - 183
Copyright
Copyright © International Astronomical Union 2013 

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