Dear all,
here is the arxiv link to a new paper that has just been published on ApJ Letters http://arxiv.org/abs/1204.0041 The paper addresses diagnostics of hot plasma using AIA data and validating the method with simultaneous EIS spectroscopic data. Please find the title and abstract below.
cheers, Paola
"Hinode/EIS spectroscopic validation of very hot plasma imaged with Solar Dynamics Observatory in non-flaring active region cores"
Testa P. & Reale F.
Abstract: We use coronal imaging observations with SDO/AIA, and Hinode/EIS spectral data, to explore the potential of narrow band EUV imaging data for diagnosing the presence of hot (T >~ 5 MK) coronal plasma in active regions. We analyze observations of two active regions (AR 11281, AR 11289) with simultaneous AIA imaging, and EIS spectral data, including the Ca xvii line (at 192.8A) which is one of the few lines in the EIS spectral bands sensitive to hot coronal plasma even outside flares. After careful coalignment of the imaging and spectral data, we compare the morphology in a 3 color image combining the 171, 335, and 94A AIA spectral bands, with the image obtained for Ca xvii emission from the analysis of EIS spectra. We find that in the selected active regions the Ca xvii emission is strong only in very limited areas, showing striking similarities with the features bright in the 94A (and 335A) AIA channels and weak in the 171A band. We conclude that AIA imaging observations of the solar corona can be used to track hot plasma (6-8 MK), and so to study its spatial variability and temporal evolution at high spatial and temporal resolution.