Is the Polar Region Different from the Quiet Region of the Sun?
Hiroaki Ito, Saku Tsuneta, Daikou Shiota, Munetoshi Tokumaru, Ken'ichi, Fujiki

TL;DR
This study compares the magnetic properties of the Sun's polar region and quiet Sun, revealing larger magnetic flux and predominantly open magnetic field lines in the polar region, which are crucial for understanding solar dynamics.
Contribution
It provides detailed magnetic field measurements of the polar region versus quiet Sun, highlighting differences in flux, polarity, and magnetic topology using Hinode observations.
Findings
Polar region has larger magnetic flux than quiet Sun.
Magnetic field lines in the polar region are mostly open.
Horizontal magnetic fields are similar in both regions.
Abstract
Observations of the polar region of the Sun are critically important for understanding the solar dynamo and the acceleration of solar wind. We carried out precise magnetic observations on both the North polar region and the quiet Sun at the East limb with the Spectro-Polarimeter of the Solar Optical Telescope aboard Hinode to characterize the polar region with respect to the quiet Sun. The average area and the total magnetic flux of the kG magnetic concentrations in the polar region appear to be larger than those of the quiet Sun. The magnetic field vectors classified as vertical in the quiet Sun have symmetric histograms around zero in the strengths, showing balanced positive and negative flux, while the histogram in the North polar region is clearly asymmetric, showing a predominance of the negative polarity. The total magnetic flux of the polar region is larger than that of the quiet…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Geomagnetism and Paleomagnetism Studies · Geophysics and Gravity Measurements
