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Defining the Middle Corona
DOI: 10.1007/s11207-023-02170-1 Bibcode: 2023SoPh..298...78W

Giordano, Silvio; Andretta, Vincenzo; Reeves, Katharine K. +39 more

The middle corona, the region roughly spanning heliocentric distances from 1.5 to 6 solar radii, encompasses almost all of the influential physical transitions and processes that govern the behavior of coronal outflow into the heliosphere. The solar wind, eruptions, and flows pass through the region, and they are shaped by it. Importantly, the reg…

2023 Solar Physics
PROBA-2 SOHO 32
Rapid Rotation of an Erupting Prominence and the Associated Coronal Mass Ejection on 13 May 2013
DOI: 10.1007/s11207-023-02126-5 Bibcode: 2023SoPh..298...35Z

Zhang, Qingmin; Ji, Haisheng; Zhou, Yuhao

In this paper, we report the multiwavelength observations of an erupting prominence and the associated coronal mass ejection (CME) on 13 May 2013. The event occurs behind the western limb in the field of view of the Atmospheric Imaging Assembly (AIA) on board the Solar Dynamics Observatory (SDO) spacecraft. The prominence is supported by a highly …

2023 Solar Physics
PROBA-2 SOHO 8
The SWAP Filter: A Simple Azimuthally Varying Radial Filter for Wide-Field EUV Solar Images
DOI: 10.1007/s11207-023-02183-w Bibcode: 2023SoPh..298...92S

Berghmans, David; Rachmeler, Laurel A.; West, Matthew J. +5 more

We present the SWAP Filter: an azimuthally varying, radial normalizing filter specifically developed for EUV images of the solar corona, named for the Sun Watcher with Active Pixels and Image Processing (SWAP) instrument on the Project for On-Board Autonomy 2 (PROBA2) spacecraft. We discuss the origins of our technique, its implementation and key …

2023 Solar Physics
PROBA-2 3