A Statistical Analysis of the Solar Phenomena Associated with Global EUV Waves
arXiv:1711.02530 · doi:10.1007/s11207-017-1206-0
Abstract
Solar eruptions are the most spectacular events in our solar system and are associated with many different signatures of energy release including solar flares, coronal mass ejections, global waves, radio emission and accelerated particles. Here, we apply the Coronal Pulse Identification and Tracking Algorithm (CorPITA) to the high cadence synoptic data provided by the Solar Dynamic Observatory (SDO) to identify and track global waves observed by SDO. 164 of the 362 solar flare events studied (45%) are found to have associated global waves with no waves found for the remaining 198 (55%). A clear linear relationship was found between the median initial velocity and the acceleration of the waves, with faster waves exhibiting a stronger deceleration (consistent with previous results). No clear relationship was found between global waves and type II radio bursts, electrons or protons detected in-situ near Earth. While no relationship was found between the wave properties and the associated flare size (with waves produced by flares from B to X-class), more than a quarter of the active regions studied were found to produce more than one wave event. These results suggest that the presence of a global wave in a solar eruption is most likely determined by the structure and connectivity of the erupting active region and the surrounding quiet solar corona rather than by the amount of free energy available within the active region.
33 pages, 6 figures, 1 table. Accepted for publication in Solar Physics
References in corpus (8)
- Advances in Observing Various Coronal EUV Waves in the SDO Era and Their Seismological Applications (Invited Review)
- The formation heights of coronal shocks from 2D density and Alfvén speed maps
- Off-limb Solar Coronal Wavefronts From SDO/AIA EUV Observations - Implications For Particle Production
- Understanding the Physical Nature of Coronal "EIT Waves"
- Statistical Analysis of Large-scale EUV Waves Observed by STEREO/EUVI
- CorPITA: An Automated Algorithm for the Identification and Analysis of Coronal "EIT Waves"
- The Relation Between Large-Scale Coronal Propagating Fronts and Type II Radio Bursts
- Radio Bursts Associated with Flare and Ejecta in the 13 July 2004 Event
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