Solar-Cycle Variation of quiet-Sun Magnetism and Surface Gravity Oscillation Mode

Abstract

The origin of the quiet Sun magnetism is under debate. Investigating the solar cycle variation observationally in more detail can give us clues about how to resolve the controversies. We investigate the solar cycle variation of the most magnetically quiet regions and their surface gravity oscillation ($f$-) mode integrated energy ($E_f$). We use 12 years of HMI data and apply a stringent selection criteria, based on spatial and temporal quietness, to avoid any influence of active regions (ARs). We develop an automated high-throughput pipeline to go through all available magnetogram data and to compute $E_f$ for the selected quiet regions. We observe a clear solar cycle dependence of the magnetic field strength in the most quiet regions containing several supergranular cells. For patch sizes smaller than a supergranular cell, no significant cycle dependence is detected. The $E_f$ at the supergranular scale is not constant over time. During the late ascending phase of Cycle 24 (SC24, 2011-2012), it is roughly constant, but starts diminishing in 2013, as the maximum of SC24 is approached. This trend continues until mid-2017, when hints of strengthening at higher southern latitudes are seen. Slow strengthening continues, stronger at higher latitudes than at the equatorial regions, but $E_f$ never returns back to the values seen in 2011-2012. Also, the strengthening trend continues past the solar minimum, to the years when SC25 is already clearly ascending. Hence the $E_f$ behavior is not in phase with the solar cycle. The anticorrelation of $E_f$ with the solar cycle in gross terms is expected, but the phase shift of several years indicates a connection to the poloidal large-scale magnetic field component rather than the toroidal one. Calibrating AR signals with the QS $E_f$ does not reveal significant enhancement of the $f$-mode prior to AR emergence.

arXiv comment10 pages, 11 figures, submitted to Astronomy & Astrophysics

References in corpus (15)

• Astropy: A Community Python Package for Astronomy
• Binary companions of evolved stars in APOGEE DR14: Search method and catalog of ~5,000 companions
• Astrophysical magnetic fields and nonlinear dynamo theory
• The Helioseismic and Magnetic Imager (HMI) Vector Magnetic Field Pipeline: Overview and Performance
• Observables Processing for the Helioseismic and Magnetic Imager Instrument on the Solar Dynamics Observatory
• Quiet Sun magnetic fields observed by Hinode: Support for a local dynamo
• Two-scale analysis of solar magnetic helicity
• On-Orbit Performance of the Helioseismic and Magnetic Imager Instrument onboard the Solar Dynamics Observatory
• Bihelical spectrum of solar magnetic helicity and its evolution
• Solar chromospheric emission and magnetic structures from plages to intranetwork: Contribution of the very quiet Sun
• High-wavenumber solar $f$-mode strengthening prior to active region formation
• Fanning out of the $f$-mode in presence of nonuniform magnetic fields
• Properties of $p$- and $f$-modes in hydromagnetic turbulence
• $f$-mode strengthening from a localized bipolar subsurface magnetic field
• Magnetic flux structuring of the quiet Sun internetwork. Center-to-limb analysis of solar-cycle variations