Flares are localized phenomena in active regions, but the magnetic and plasma responses may propagate to a larger area. In this work we investigate the temporal evolution of a flare in an active region with particular attention to the morphological details, and to the temperature and emission measure diagnostics allowed by Hinode/XRT.

Parenti, S., Reale, F., Reeves, K.K. (2012). Plasma Diagnostics and Magnetic Complexity of a Post-Flare Active Region with Hinode/XRT: Spatial and Temporal Evolution. In Hinode-3: The 3rd Hinode Science Meeting (pp.291-294). San Francisco : Astronomical Society of the Pacific.

Plasma Diagnostics and Magnetic Complexity of a Post-Flare Active Region with Hinode/XRT: Spatial and Temporal Evolution

REALE, Fabio;
2012-01-01

Abstract

Flares are localized phenomena in active regions, but the magnetic and plasma responses may propagate to a larger area. In this work we investigate the temporal evolution of a flare in an active region with particular attention to the morphological details, and to the temperature and emission measure diagnostics allowed by Hinode/XRT.
Settore FIS/05 - Astronomia E Astrofisica
Hinode-3: The 3rd Hinode Science Meeting
Tokyo, Japan
1-4 December 2009
2012
4
http://aspbooks.org/custom/publications/paper/454-0291.html
Parenti, S., Reale, F., Reeves, K.K. (2012). Plasma Diagnostics and Magnetic Complexity of a Post-Flare Active Region with Hinode/XRT: Spatial and Temporal Evolution. In Hinode-3: The 3rd Hinode Science Meeting (pp.291-294). San Francisco : Astronomical Society of the Pacific.
Proceedings (atti dei congressi)
Parenti, S; Reale, F; Reeves, KK
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/10447/73220
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