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Multi-Scale Gaussian Normalization for Solar Image Processing
DOI: 10.1007/s11207-014-0523-9 Bibcode: 2014SoPh..289.2945M

Morgan, Huw; Druckmüller, Miloslav

Extreme ultra-violet images of the corona contain information over a wide range of spatial scales, and different structures such as active regions, quiet Sun, and filament channels contain information at very different brightness regimes. Processing of these images is important to reveal information, often hidden within the data, without introduci…

2014 Solar Physics
PROBA-2 SOHO 180
Bridging EUV and White-Light Observations to Inspect the Initiation Phase of a "Two-Stage" Solar Eruptive Event
DOI: 10.1007/s11207-014-0585-8 Bibcode: 2014SoPh..289.4545B

Seaton, D. B.; Habbal, S. R.; Bain, H. M. +2 more

The initiation phase of coronal mass ejections (CMEs) is a very important aspect of solar physics, as these phenomena ultimately drive space weather in the heliosphere. This phase is known to occur between the photosphere and low corona, where many models introduce an instability and/or magnetic reconnection that triggers a CME, often with associa…

2014 Solar Physics
PROBA-2 SOHO 31
Coronal Mass Ejections Observed at the Total Solar Eclipse on 13 November 2012
DOI: 10.1007/s11207-014-0476-z Bibcode: 2014SoPh..289.2587H

Hanaoka, Yoichiro; Nakazawa, Jun; Ohgoe, Osamu +2 more

White-light observations of the total solar eclipse on 13 November 2012 were made at two sites, where the totality occurred 35 min apart. The structure of the corona from the solar limb to a couple of solar radii was observed with a wide dynamic range and a high signal-to-noise ratio. An ongoing coronal mass ejection (CME) and a pre-CME loop struc…

2014 Solar Physics
PROBA-2 SOHO 13