Calendar

Jan
10
Wed
riunione su HR 9024 (Argiroffi)
Jan 10 @ 15:30 – 17:30
Jan
15
Mon
PRIN – MIUR
Jan 15 @ 11:00 – 13:30
Jan
17
Wed
Riunione SCN @ aula, Osservatorio
Jan 17 @ 11:30 – 13:00
Jan
24
Wed
Riunione divulgazione @ aula, Osservatorio
Jan 24 @ 11:00 – 13:00
Jan
26
Fri
Riunione museo
Jan 26 @ 11:00 – 13:00
Feb
7
Wed
riunione gruppo di lavoro “gestione documentale”
Feb 7 @ 14:30 – 18:00

Genco Russo – Martines – Morale

Feb
12
Mon
ASTROSMART esami orali
Feb 12 – Feb 13 all-day
Feb
15
Thu
Riunione gruppo SNR
Feb 15 @ 11:00 – 13:30

Riunione gruppo SNR

Il cielo dell’altra metà del cielo: breve storia del contributo delle donne in astronomia seminario di Ileana Chinnici) @ Osservatorio Astroomico di Palermo
Feb 15 @ 15:30 – 17:00

Il talk presenterà alcune figure femminili che hanno contribuito allo sviluppo della scienza astronomica, dalle origini al XX secolo, sottolineando alcuni aspetti che hanno favorito il loro approccio all’astronomia e alcune caratteristiche tipiche del loro contributo.

Ileana Chinnici (INAF – Osservatorio Astronomico di Palermo)

Feb
19
Mon
Properties of solar coronal heating in active regions, from high resolution spectroscopy. Paola Testa (Smithsonian Astrophysical Observatory, USA)
Feb 19 @ 11:00 – 12:30

Abstract.

I will discuss how high spatial, spectral, and temporal resolution chromospheric/transition region/coronal observations coupled with detailed modeling can help us diagnose coronal heating properties in active region cores in non-flaring conditions.  I will focus on recent results from the Interface Region Imaging Spectrograph (IRIS), which provides us with unprecedented high spatial, temporal and spectral resolution observations of the chromosphere and transition region. Joint with coronal observations with Hinode (XRT and EIS), and SDO/AIA, these data cover from the upper photosphere to the corona.

In particular, I will discuss how IRIS observations of footpoints of hot active region loops, coupled with detailed HD and MHD modeling including chromosphere, transition region and corona, provide tight constraints on the coronal heating mechanisms in the core of active regions.