8th Coronal Loops Workshop:

many facets of magnetically closed corona

Grand Hotel Piazza Borsa, Palermo Italy

27-30 June 2017


E-posters PROCEEDINGS

Ugarte-Urra - Modeling Coronal Response in Decaying Active Regions with Magnetic Flux Transport and Steady Heating

Graham - Automated detection of transient moss features

Li - Some progresses for space observations of solar corona from China, instrument overview

Tajfirouze - EUV flickering of solar coronal loops

Wright - Thermal Time Evolution of Non-Flaring Active Regions Determined by SDO/AIA

Kirichenko - Plasma heating in solar microflares during the minimum of solar activity

Reva - Absence of the hot plasma in non-flaring active regions + Video

Gudiksen - Identifying heating events in the corona

Downs - Characterizing the Observational Signatures of Coronal Heating Models for Realistic Magnetic Fields and Lines-of-Sight

Klimchuk - Conditions Necessary for Thermal Non-equilibrium + videos (avi and mpg)

Lorincik - Diagnostics of non-Maxwellian κ-distributions in Hinode/EIS active region spectral atlas

Lionello - Fully 3D Modeling of Prominence Formation by Plasma Evaporation and Condensation

Andretta - The contribution of type II spicules to the transition region radiative output

Shestov -  ASPIICS spaceborne coronagraph

Drake - Suppression of CMEs on Active Stars by Overlying Magnetic Field