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Multipoint Study of Successive Coronal Mass Ejections Driving Moderate Disturbances at 1 au
DOI: 10.3847/1538-4357/ab1850 Bibcode: 2019ApJ...878...37P

Poedts, Stefaan; Scolini, Camilla; West, Matthew J. +10 more

We analyze in this work the propagation and geoeffectiveness of four successive coronal mass ejections (CMEs) that erupted from the Sun during 2013 May 21-23 and were detected in interplanetary space by the Wind and/or STEREO-A spacecraft. All these CMEs featured critical aspects for understanding so-called “problem space weather storms” at Earth.…

2019 The Astrophysical Journal
PROBA-2 SOHO 29
Comprehensive Analysis of the Formation of a Shock Wave Associated with a Coronal Mass Ejection
DOI: 10.3847/1538-4357/aaf9af Bibcode: 2019ApJ...871..212F

Susino, Roberto; Frassati, Federica; Mancuso, Salvatore +1 more

On 2014 November 1, a solar prominence eruption associated with a C2.7 class flare and a type II radio burst resulted in a fast partial halo coronal mass ejection (CME). Images acquired in the extreme ultraviolet (EUV) by the Solar Dynamics Observatory/Atmospheric Imaging Assembly (AIA) and PROBA2/SWAP and in white light (WL) by Solar and Heliosph…

2019 The Astrophysical Journal
PROBA-2 SOHO 24
Evolution of the Coronal Cavity From the Quiescent to Eruptive Phase Associated with Coronal Mass Ejection
DOI: 10.3847/1538-4357/ab11c5 Bibcode: 2019ApJ...875..101S

West, Matthew J.; Srivastava, Nandita; Mierla, Marilena +2 more

We present the evolution of a coronal cavity encompassing its quiescent and eruptive phases in the lower corona. Using multiple vantage-point observations from the SDO/AIA, STEREO SECCHI/EUVI, and PROBA2/Sun Watcher with the APS and Image Processing (SWAP) extreme ultraviolet (EUV) imagers, we capture a sequence of quasi-static equilibria of the q…

2019 The Astrophysical Journal
PROBA-2 SOHO 18
On the Source Position and Duration of a Solar Type III Radio Burst Observed by LOFAR
DOI: 10.3847/1538-4357/ab458f Bibcode: 2019ApJ...885..140Z

Kontar, Eduard P.; Zhang, PeiJin; Yu, SiJie +1 more

The flux of solar type III radio bursts have a time profile of rising and decay phases at a given frequency, which has been actively studied since the 1970s. Several factors that may influence the duration of a type III radio burst have been proposed. In this work, to study the dominant cause of the duration, we investigate the source positions of…

2019 The Astrophysical Journal
PROBA-2 14
Exceptional Extended Field-of-view Observations by PROBA2/SWAP on 2017 April 1 and 3
DOI: 10.3847/1538-4357/ab3b08 Bibcode: 2019ApJ...883...59O

West, Matthew J.; Mierla, Marilena; D'Huys, Elke +2 more

On 2017 April 1 and 3, two large eruptions on the western solar limb, which were associated with M4.4- and M5.8-class flares, respectively, were observed with the Sun Watcher with Active Pixels and Image Processing (SWAP) Extreme Ultraviolet (EUV) solar telescope on board the Project for On Board Autonomy 2 (PROBA2) spacecraft. The large field-of-…

2019 The Astrophysical Journal
PROBA-2 SOHO 14