ASSOCIATION OF {sup 3}He-RICH SOLAR ENERGETIC PARTICLES WITH LARGE-SCALE CORONAL WAVES

• Published in: The Astrophysical journal Vol. 833; no. 1
• Main Authors: Bučík, Radoslav, Innes, Davina E., Mason, Glenn M., Wiedenbeck, Mark E.
• Format: Journal Article
• Language: English
• Published: United States 10.12.2016
• Subjects: ACCELERATION; ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; EXTREME ULTRAVIOLET RADIATION; FRACTIONATION; HELIUM 3; INTERPLANETARY SPACE; JETS; MAGNETIC FIELDS; MAGNETIC RECONNECTION; MASS; RESOLUTION; SHOCK WAVES; SOLAR CORONA; SOLAR FLARES; SUN
• ISSN: 0004-637X; 1538-4357
• DOI: 10.3847/1538-4357/833/1/63

Small, {sup 3}He-rich solar energetic particle (SEP) events have been commonly associated with extreme-ultraviolet (EUV) jets and narrow coronal mass ejections (CMEs) that are believed to be the signatures of magnetic reconnection, involving field lines open to interplanetary space. The elemental and isotopic fractionation in these events are thought to be caused by processes confined to the flare sites. In this study, we identify 32 {sup 3}He-rich SEP events observed by the Advanced Composition Explorer , near the Earth, during the solar minimum period 2007–2010, and we examine their solar sources with the high resolution Solar Terrestrial Relations Observatory ( STEREO ) EUV images. Leading the Earth, STEREO -A has provided, for the first time, a direct view on {sup 3}He-rich flares, which are generally located on the Sun’s western hemisphere. Surprisingly, we find that about half of the {sup 3}He-rich SEP events in this survey are associated with large-scale EUV coronal waves. An examination of the wave front propagation, the source-flare distribution, and the coronal magnetic field connections suggests that the EUV waves may affect the injection of {sup 3}He-rich SEPs into interplanetary space.