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. (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.
File in questo prodotto:
| File | Dimensione | Formato | |
|---|---|---|---|
|
291.pdf
Solo gestori archvio
Descrizione: main article
Tipologia:
Versione Editoriale
Dimensione
538.16 kB
Formato
Adobe PDF
|
538.16 kB | Adobe PDF | Visualizza/Apri Richiedi una copia |
I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
