Magnetic Helicity Flux across Solar Active Region Photospheres. II. Association of Hemispheric Sign Preference with Flaring Activity during Solar Cycle 24
نویسندگان
چکیده
In our earlier study of this series (Park et al. 2020, Paper I), we examined the hemispheric sign preference (HSP) magnetic helicity flux $dH/dt$ across photospheric surfaces 4802 samples 1105 unique active regions (ARs) observed during solar cycle 24. Here, investigate any association HSP, expressed as a degree compliance, with flaring activity, analyzing same set estimates used in I. The AR under investigation are assigned to heliographic (HRs) defined Carrington longitude-latitude plane grid spacing 45$^\circ$ longitude and 15$^\circ$ latitude. For each HRs, calculate HSP compliance average soft X-ray flare index. strongest activity is found be one distinctive HR an extremely low 41% compared mean standard deviation 62% 7%, respectively, over all HRs. This sole shows anti-HSP (i.e., less than 50%) includes highly flare-productive NOAA 12673, however not uniquely responsible for HR's HSP. We also find that HRs highest located southern hemisphere, they tend have lower degrees compliance. These findings point presence localized convection zone enhanced turbulence, imparting greater complexity higher rate some rising tubes.
منابع مشابه
Solar Active Region Flux Fragmentation, Subphotospheric Flows, and Flaring
We explore the properties of the fragmentation of magnetic flux in solar active regions. We apply gradient-based tessellation to magnetograms of 59 active regions to identify flux fragments. First, we find that the distribution function of flux fragments in these regions is highly consistent with lognormal form, which is the most direct evidence yet obtained that repeated random bifurcation dom...
متن کاملMagnetic Helicity, Coronal Heating and Solar Flaring Activity: A Review of the Role of Active Region Twist
Magnetic helicity of solar active regions is quantified by the twist and writhe of their underlying flux tubes. The twist component, in particular, is believed to be an important determinant of the energetics and dynamics of active regions that ultimately lead to coronal heating and solar eruptive activity. Here, I review the role of active region twist in the context of solar activity – laying...
متن کاملMagnetic Helicity and Energy Spectra of a Solar Active Region
We compute magnetic helicity and energy spectra of the solar active region NOAA 11158 during 11–15 February 2011 at 20 southern heliographic latitude using observational photospheric vector magnetograms. We adopt the isotropic representation of the Fourier-transformed two-point correlation tensor of the magnetic field. The sign of magnetic helicity turns out to be predominantly positive at all ...
متن کاملMagnetic helicity evolution during the solar activity cycle: observations and dynamo theory
We study a simple model for the solar dynamo in the framework of the Parker migratory dynamo, with a nonlinear dynamo saturation mechanism based on magnetic helicity conservation arguments. We find a parameter range in which the model demonstrates a cyclic behaviour with properties similar to that of Parker dynamo with the simplest form of algebraic α-quenching. We compare the nonlinear current...
متن کاملStudy of Magnetic Helicity in Solar Active Regions and Its Relationship with Solar Eruptions
STUDY OF MAGNETIC HELICITY IN SOLAR ACTIVE REGIONS AND ITS RELATIONSHIP WITH SOLAR ERUPTIONS by Sung-Hong Park It is generally believed that eruptive phenomena in the solar atmosphere such as solar flares and coronal mass ejections (CMEs) occur in solar active regions with complex magnetic structures. The magnetic complexity is quantified in terms of twists, kinks, and interlinkages of magnetic...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
ژورنال
عنوان ژورنال: The Astrophysical Journal
سال: 2021
ISSN: ['2041-8213', '2041-8205']
DOI: https://doi.org/10.3847/1538-4357/abea13