Major solar eruptions and high-energy particle events during solar cycle 24

被引:0
作者
Nat Gopalswamy
Hong Xie
Sachiko Akiyama
Pertti A Mäkelä
Seiji Yashiro
机构
[1] NASA Goddard Space Flight Center,
[2] The Catholic University of America,undefined
来源
Earth, Planets and Space | / 66卷
关键词
Coronal mass ejections; Flares; Ground level enhancement events; Solar energetic particle events;
D O I
暂无
中图分类号
学科分类号
摘要
We report on a study of all major solar eruptions that occurred on the frontside of the Sun during the rise to peak phase of cycle 24 (first 62 months) in order to understand the key factors affecting the occurrence of large solar energetic particle events (SEPs) and ground level enhancement (GLE) events. The eruptions involve major flares with soft X-ray peak flux ≥ 5.0 x10−5 Wm−2 (i.e., flare size ≥ M5.0) and accompanying coronal mass ejections (CMEs). The selection criterion was based on the fact that the only front-side GLE in cycle 24 (GLE 71) had a flare size of M5.1. Only approximately 37% of the major eruptions from the western hemisphere resulted in large SEP events. Almost the same number of large SEP events was produced in weaker eruptions (flare size < M5.0), suggesting that the soft X-ray flare is not a good indicator of SEP or GLE events. On the other hand, the CME speed is a good indicator of SEP and GLE events because it is consistently high supporting the shock acceleration mechanism. We found the CME speed, magnetic connectivity to Earth (in longitude and latitude), and ambient conditions as the main factors that contribute to the lack of high-energy particle events during cycle 24. Several eruptions poorly connected to Earth (eastern-hemisphere or behind-the-west-limb events) resulted in very large SEP events detected by the Solar Terrestrial Relations Observatory (STEREO) spacecraft. Some very fast CMEs, likely to have accelerated particles to GeV energies, did not result in a GLE event because of poor latitudinal connectivity. The stringent latitudinal requirement suggests that the highest-energy particles are likely accelerated in the nose part of shocks, while the lower energy particles are accelerated at all parts. There were also well-connected fast CMEs, which did not seem to have accelerated high-energy particles due to possible unfavorable ambient conditions (high Alfven speed, overall reduction in acceleration efficiency in cycle 24).
引用
收藏
相关论文
共 50 条
[21]   Characterizing High-Energy Solar Proton Events with Energies Below and Above 100 MeV [J].
Ameri, Dheyaa ;
Valtonen, Eino ;
Al-Sawad, Amjad ;
Vainio, Rami .
SOLAR PHYSICS, 2024, 299 (09)
[22]   High-Speed Solar Wind Streams and Geomagnetic Storms During Solar Cycle 24 [J].
Gerontidou, M. ;
Mavromichalaki, H. ;
Daglis, T. .
SOLAR PHYSICS, 2018, 293 (09)
[23]   High-Speed Solar Wind Streams and Geomagnetic Storms During Solar Cycle 24 [J].
M. Gerontidou ;
H. Mavromichalaki ;
T. Daglis .
Solar Physics, 2018, 293
[24]   Forecasting Solar Energetic Particle Events During Solar Cycles 23 and 24 Using Interpretable Machine Learning [J].
Kasapis, Spiridon ;
Kitiashvili, Irina N. ;
Kosovich, Paul ;
Kosovichev, Alexander G. ;
Sadykov, Viacheslav M. ;
O'Keefe, Patrick ;
Wang, Vincent .
ASTROPHYSICAL JOURNAL, 2024, 974 (01)
[25]   Analysis of solar energetic particle (SEP) event on the geomagnetic environment during 24th solar cycle [J].
Kumar, Nirmal R. ;
Inbaseelan, Ranjith Dev C. ;
Karthikeyan, E. ;
Nithyasree, M. ;
Jeyakumar, Johnson H. .
ASTROPHYSICS AND SPACE SCIENCE, 2024, 369 (06)
[26]   Major Solar Energetic Particle Events of Solar Cycles 22 and 23: Intensities Close to the Streaming Limit [J].
D. Lario ;
A. Aran ;
R. B. Decker .
Solar Physics, 2009, 260 :407-421
[27]   Particle Acceleration and Propagation in Strong Flares without Major Solar Energetic Particle Events [J].
Klein, K. -L. ;
Trottet, G. ;
Samwel, S. ;
Malandraki, O. .
SOLAR PHYSICS, 2011, 269 (02) :309-333
[28]   Major Solar Energetic Particle Events of Solar Cycles 22 and 23: Intensities Close to the Streaming Limit [J].
Lario, D. ;
Aran, A. ;
Decker, R. B. .
SOLAR PHYSICS, 2009, 260 (02) :407-421
[29]   Analysis of Geoeffective Impulsive Events on the Sun During the First Half of Solar Cycle 24 [J].
Agnieszka Gil ;
Monika Berendt-Marchel ;
Renata Modzelewska ;
Agnieszka Siluszyk ;
Marek Siluszyk ;
Anna Wawrzaszek ;
Anna Wawrzynczak .
Solar Physics, 2023, 298
[30]   3He-rich Events During the Rising Phase of Solar Cycle 24 [J].
Ho, George C. ;
Mason, Glenn M. .
OUTSTANDING PROBLEMS IN HELIOPHYSICS: FROM CORONAL HEATING TO THE EDGE OF THE HELIOSPHERE, 2014, 484 :72-77