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Investigating coronal heating from new high resolution solar observations: Hi-C (and IRIS) | Paola Testa (Smithsonian Astrophysical Observatory – USA)
@ Aula OAPA
Investigating coronal heating from new high resolution solar observations: Hi-C (and IRIS) | Paola Testa (Smithsonian Astrophysical Observatory – USA)
@ Aula OAPA
Jun 21 @ 12:00 – 13:00
The Hi-C (High resolution Coronal imager) sounding rocket has provided the highest resolution EUV solar coronal images ever obtained, resolving structures down to ~0.3 arcsec. The unprecedented spatial and temporal resolution of Hi-C data has revealed several new features, including highly braided coronal loops undergoing reconnection, and very rapid variability (down to ~15s) in the moss of bright hot loops.
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