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Coronal Dimmings and the Early Phase of a CME Observed with STEREO and Hinode/EIS

Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
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Coronal ejections from convective spherical shell dynamos

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Coronal Electron Distribution in Solar Flares: Drift-Kinetic Model

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Coronal emission lines as thermometers

Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
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Coronal Fe XIV Emission During the Whole Heliosphere Interval Campaign

Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
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Coronal fuzziness modelled with pulse-heated multistranded loop systems

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Coronal heating in coupled photosphere-chromosphere-coronal systems: turbulence and leakage

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Coronal hole boundaries evolution at small scales: I. EIT 195 A and TRACE 171 A view

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Coronal hole boundaries evolution at small scales: II. XRT view Can small-scale outflows at CHBs be a source of the slow solar wind?

Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
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Coronal Holes

Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
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Coronal Implosion and Particle Acceleration in the Wake of a Filament Eruption

Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
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Coronal Inflows and Giant Polar Plumes

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Coronal Loop Expansion Properties Explained Using Separators

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Coronal Loop Models and Those Annoying Observations!

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Coronal Loop Oscillations Observed with AIA - Kink-Mode with Cross-Sectional and Density Oscillations

Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
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Coronal Loops: Observations and Modeling of Confined Plasma

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Coronal Magnetic Field Measurement from EUV Images made by the Solar Dynamics Observatory

Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
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Coronal Magnetic Field Structure and Evolution for Flaring AR 11117 and its Surroundings

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Coronal Mass Ejection Detection using Wavelets, Curvelets and Ridgelets: Applications for Space Weather Monitoring

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Coronal mass ejection initiation: On the nature of the Flux Cancellation Model

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