2016/12/04 by Yan Ouyang, Y. Ouyang, Y. H. Zhou +4 · 2 citations
Chemistry · Computer Science · Mathematics · Physics and Astronomy · #Astro and Planetary Science #Astrophysics #Chemistry #Chirality (physics) #Fault (geology) #Geology #Helicity #Magnetic field #Magnetic helicity #Materials science #Mathematics #Paleontology #Phase (matter) #Physics #Polarity (international relations) #Protein filament #Quantum mechanics #Rope #Sinistral and dextral #Solar Radiation and Photovoltaics #Solar and Space Plasma Dynamics #astro-ph.SR
paper · pdf · doi:10.3847/1538-4357/835/1/94
15 pages, 5 figures, accepted for publication in ApJ
arxiv created 2016/12/04 · openalex publication_date 2017/01/20 · arxiv updated 2017/01/25 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
ABSTRACT It has been revealed that the magnetic topology in the solar atmosphere displays hemispheric preference, i.e., helicity is mainly negative/positive in the northern/southern hemispheres, respectively. However, the strength of the hemispheric rule and its cyclic variation are controversial. In this paper, we apply a new method based on the filament drainage to 571 erupting filaments from 2010 May to 2015 December in order to determine the filament chirality and its hemispheric preference. It is found that 91.6% of our sample of erupting filaments follows the hemispheric rule of helicity sign. It is also found that the strength of the hemispheric preference of the quiescent filaments decreases slightly from ∼97% in the rising phase to ∼85% in the declining phase of solar cycle 24, whereas the strength of the intermediate filaments keeps a high value around 96 ± 4% at all times. Only the active-region filaments show significant variations. Their strength of the hemispheric rule rises from ∼63% to ∼95% in the rising phase, and keeps a high value of 82% ± 5% during the declining phase. Furthermore, during a half-year period around the solar maximum, their hemispheric preference totally vanishes. Additionally, we also diagnose the magnetic configurations of the filaments based on our indirect method and find that in our sample of erupting events, 89% are inverse-polarity filaments with a flux rope magnetic configuration, whereas 11% are normal-polarity filaments with a sheared arcade configuration.