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Properties of solar coronal heating in active regions, from high resolution spectroscopy. Paola Testa (Smithsonian Astrophysical Observatory, USA)
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
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