Recent spatial solar missions, such as Hinode and Solar Dynamics Observatory, reveal a more and more highly structured and dynamic corona, with an increasing importance and debate. The connection of structure and dynamics to coronal heating is fundamental. Observations and evidence of fine coronal structuring, e.g. moss and emission measure distributions, and dynamics, e.g. Doppler shifts, spicules, are discussed and compared to current vision and models. Open questions and future perspectives are outlined to conclude.
Reale, F. (2012). Coronal structure and dynamics. In 39th COSPAR Scientific Assembly (pp.1596-1596).
Coronal structure and dynamics
REALE, Fabio
2012-01-01
Abstract
Recent spatial solar missions, such as Hinode and Solar Dynamics Observatory, reveal a more and more highly structured and dynamic corona, with an increasing importance and debate. The connection of structure and dynamics to coronal heating is fundamental. Observations and evidence of fine coronal structuring, e.g. moss and emission measure distributions, and dynamics, e.g. Doppler shifts, spicules, are discussed and compared to current vision and models. Open questions and future perspectives are outlined to conclude.
File in questo prodotto:
| File | Dimensione | Formato | |
|---|---|---|---|
|
E2.1-0010-12.pdf
accesso aperto
Descrizione: abstract text
Dimensione
23.42 kB
Formato
Adobe PDF
|
23.42 kB | Adobe PDF | Visualizza/Apri |
I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
