Literature DB >> 27194965

Magnetic Structure of Sunspots.

Juan M Borrero1, Kiyoshi Ichimoto2.   

Abstract

In this review we give an overview about the current state-of-knowledge of the magnetic field in sunspots from an observational point of view. We start by offering a brief description of tools that are most commonly employed to infer the magnetic field in the solar atmosphere with emphasis in the photosphere of sunspots. We then address separately the global and local magnetic structure of sunspots, focusing on the implications of the current observations for the different sunspots models, energy transport mechanisms, extrapolations of the magnetic field towards the corona, and other issues. ELECTRONIC SUPPLEMENTARY MATERIAL: Supplementary material is available for this article at 10.12942/lrsp-2011-4.

Year:  2011        PMID: 27194965      PMCID: PMC4841203          DOI: 10.12942/lrsp-2011-4

Source DB:  PubMed          Journal:  Living Rev Sol Phys        ISSN: 1614-4961            Impact factor:   17.417


  11 in total

1.  Anomalous polarization profiles in sunspots: possible origin of umbral flashes

Authors: 
Journal:  Science       Date:  2000-05-26       Impact factor: 47.728

2.  Downward pumping of magnetic flux as the cause of filamentary structures in sunspot penumbrae.

Authors:  John H Thomas; Nigel O Weiss; Steven M Tobias; Nicholas H Brummell
Journal:  Nature       Date:  2002-11-28       Impact factor: 49.962

3.  Dark cores in sunspot penumbral filaments.

Authors:  Göran B Scharmer; Boris V Gudiksen; Dan Kiselman; Mats G Löfdahl; Luc H M Rouppe van der Voort
Journal:  Nature       Date:  2002-11-14       Impact factor: 49.962

4.  Three-dimensional magnetic field topology in a region of solar coronal heating.

Authors:  S K Solanki; A Lagg; J Woch; N Krupp; M Collados
Journal:  Nature       Date:  2003-10-16       Impact factor: 49.962

5.  Zero-field dichroism in the solar chromosphere.

Authors:  R Manso Sainz; J Trujillo Bueno
Journal:  Phys Rev Lett       Date:  2003-09-09       Impact factor: 9.161

6.  Small-scale jetlike features in penumbral chromospheres.

Authors:  Y Katsukawa; T E Berger; K Ichimoto; B W Lites; S Nagata; T Shimizu; R A Shine; Y Suematsu; T D Tarbell; A M Title; S Tsuneta
Journal:  Science       Date:  2007-12-07       Impact factor: 47.728

7.  Twisting motions of sunspot penumbral filaments.

Authors:  K Ichimoto; Y Suematsu; S Tsuneta; Y Katsukawa; T Shimizu; R A Shine; T D Tarbell; A M Title; B W Lites; M Kubo; S Nagata
Journal:  Science       Date:  2007-12-07       Impact factor: 47.728

8.  Alfven waves in the solar corona.

Authors:  S Tomczyk; S W McIntosh; S L Keil; P G Judge; T Schad; D H Seeley; J Edmondson
Journal:  Science       Date:  2007-08-31       Impact factor: 47.728

9.  Selective absorption processes as the origin of puzzling spectral line polarization from the Sun.

Authors:  J Trujillo Bueno; E Landi Degl'Innocenti; M Collados; L Merenda; R Manso Sainz
Journal:  Nature       Date:  2002-01-24       Impact factor: 49.962

10.  Penumbral structure and outflows in simulated sunspots.

Authors:  M Rempel; M Schüssler; R H Cameron; M Knölker
Journal:  Science       Date:  2009-06-18       Impact factor: 47.728

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  5 in total

1.  The source and engine of coronal mass ejections.

Authors:  Manolis K Georgoulis; Alexander Nindos; Hongqi Zhang
Journal:  Philos Trans A Math Phys Eng Sci       Date:  2019-07-01       Impact factor: 4.226

2.  Oscillations observed in umbra, plage, quiet-Sun and the polarity inversion line of active region 11158 using Helioseismic Magnetic Imager/Solar Dynamics Observatory data.

Authors:  A A Norton; R B Stutz; B T Welsch
Journal:  Philos Trans A Math Phys Eng Sci       Date:  2020-12-21       Impact factor: 4.226

Review 3.  Flare-productive active regions.

Authors:  Shin Toriumi; Haimin Wang
Journal:  Living Rev Sol Phys       Date:  2019-05-21       Impact factor: 17.417

4.  The dynamics of 3-min wavefronts and their relation to sunspot magnetic fields.

Authors:  Robert Sych; David B Jess; Jiangtao Su
Journal:  Philos Trans A Math Phys Eng Sci       Date:  2020-12-21       Impact factor: 4.226

5.  Flare differentially rotates sunspot on Sun's surface.

Authors:  Chang Liu; Yan Xu; Wenda Cao; Na Deng; Jeongwoo Lee; Hugh S Hudson; Dale E Gary; Jiasheng Wang; Ju Jing; Haimin Wang
Journal:  Nat Commun       Date:  2016-10-10       Impact factor: 14.919

  5 in total

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