Abstract

We present a visual determination of the number of bright points (BPs) existing in the quiet Sun, which are structures though to trace intense kG magnetic concentrations. The measurement is based on a 0.1 arcsec angular resolution G-band movie obtained with the Swedish Solar Telescope at the solar disk center. We find 0.97 BPs/Mm^2, which is a factor three larger than any previous estimate. It corresponds to 1.2 BPs per solar granule. Depending on the details of the segmentation, the BPs cover between 0.9% and 2.2% of the solar surface. Assuming their field strength to be 1.5 kG, the detected BPs contribute to the solar magnetic flux with an unsigned flux density between 13 G and 33 G. If network and inter-network regions are counted separately, they contain 2.2 BPs/Mm^2 and 0.85 BPs/Mm^2, respectively.

Highlights

  • As a part of this movement to characterize the properties of the quiet-Sun magnetism, we discovered the ubiquitous presence of bright points (BPs) in the intergranular lanes of the quiet Sun (Sanchez Almeida et al 2004)

  • We identify 2380 BPs, which correspond to 0.97 BPs Mm−2

  • According to the current paradigm, the BPs trace intense magnetic concentrations; so, our observation constrains the fraction of quiet-Sun plasma having kGs

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Summary

MOTIVATION

Our understanding of the quiet-Sun magnetic fields has turned over during the last decade. In agreement with the turbulent dynamo scenario, quiet-Sun magnetic fields come with strengths in the full range from basically zero to 2 kG (Sanchez Almeida & Lites 2000; Domınguez Cerdena et al 2006). Even if they only fill a small fraction of the quiet photosphere, the part having strong kG fields may be important from a physical point of view. In an effort to calibrate with visual detection one of these methods (Bovelet & Wiehr 2001, 2007), we repeated the tedious but otherwise accurate analysis carried out by Sanchez Almeida et al (2004) This time we use a G-band image of much better quality. Our density implies that the quiet Sun has more BPs than granules, and at least 1% of the quiet solar surface is covered by BPs

OBSERVATION AND ANALYSIS PROCEDURE
RESULTS
DISCUSSION
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