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Title: Distribution of electric currents in sunspots from photosphere to corona

Abstract

We present a study of two regular sunspots that exhibit nearly uniform twist from the photosphere to the corona. We derive the twist parameter in the corona and in the chromosphere by minimizing the difference between the extrapolated linear force-free field model field lines and the observed intensity structures in the extreme-ultraviolet images of the Sun. The chromospheric structures appear more twisted than the coronal structures by a factor of two. Further, we derive the vertical component of electric current density, j{sub z} , using vector magnetograms from the Hinode Solar Optical Telescope (SOT). The spatial distribution of j{sub z} has a zebra pattern of strong positive and negative values owing to the penumbral fibril structure resolved by Hinode/SOT. This zebra pattern is due to the derivative of the horizontal magnetic field across the thin fibrils; therefore, it is strong and masks weaker currents that might be present, for example, as a result of the twist of the sunspot. We decompose j{sub z} into the contribution due to the derivatives along and across the direction of the horizontal field, which follows the fibril orientation closely. The map of the tangential component has more distributed currents that are coherent with themore » chromospheric and coronal twisted structures. Moreover, it allows us to map and identify the direct and return currents in the sunspots. Finally, this decomposition of j{sub z} is general and can be applied to any vector magnetogram in order to better identify the weaker large-scale currents that are associated with coronal twisted/sheared structures.« less

Authors:
 [1];  [2];  [3]
  1. National Solar Observatory, 950 North Cherry Avenue, Tucson, AZ 85719 (United States)
  2. Observatoire de Paris, LESIA, UMR 8109 (CNRS), F-92195 Meudon Principal Cedex (France)
  3. Instituto de Astronomía y Física del Espacio (IAFE), UBA-CONICET, CC. 67, Suc. 28 Buenos Aires 1428 (Argentina)
Publication Date:
OSTI Identifier:
22365039
Resource Type:
Journal Article
Journal Name:
Astrophysical Journal
Additional Journal Information:
Journal Volume: 793; Journal Issue: 1; Other Information: Country of input: International Atomic Energy Agency (IAEA); Journal ID: ISSN 0004-637X
Country of Publication:
United States
Language:
English
Subject:
79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; CHROMOSPHERE; DECOMPOSITION; DENSITY; EXTREME ULTRAVIOLET RADIATION; IMAGES; MAGNETIC FIELDS; PHOTOSPHERE; SPATIAL DISTRIBUTION; SUN; SUNSPOTS; TELESCOPES

Citation Formats

Gosain, Sanjay, Démoulin, Pascal, and López Fuentes, Marcelo. Distribution of electric currents in sunspots from photosphere to corona. United States: N. p., 2014. Web. doi:10.1088/0004-637X/793/1/15.
Gosain, Sanjay, Démoulin, Pascal, & López Fuentes, Marcelo. Distribution of electric currents in sunspots from photosphere to corona. United States. doi:10.1088/0004-637X/793/1/15.
Gosain, Sanjay, Démoulin, Pascal, and López Fuentes, Marcelo. Sat . "Distribution of electric currents in sunspots from photosphere to corona". United States. doi:10.1088/0004-637X/793/1/15.
@article{osti_22365039,
title = {Distribution of electric currents in sunspots from photosphere to corona},
author = {Gosain, Sanjay and Démoulin, Pascal and López Fuentes, Marcelo},
abstractNote = {We present a study of two regular sunspots that exhibit nearly uniform twist from the photosphere to the corona. We derive the twist parameter in the corona and in the chromosphere by minimizing the difference between the extrapolated linear force-free field model field lines and the observed intensity structures in the extreme-ultraviolet images of the Sun. The chromospheric structures appear more twisted than the coronal structures by a factor of two. Further, we derive the vertical component of electric current density, j{sub z} , using vector magnetograms from the Hinode Solar Optical Telescope (SOT). The spatial distribution of j{sub z} has a zebra pattern of strong positive and negative values owing to the penumbral fibril structure resolved by Hinode/SOT. This zebra pattern is due to the derivative of the horizontal magnetic field across the thin fibrils; therefore, it is strong and masks weaker currents that might be present, for example, as a result of the twist of the sunspot. We decompose j{sub z} into the contribution due to the derivatives along and across the direction of the horizontal field, which follows the fibril orientation closely. The map of the tangential component has more distributed currents that are coherent with the chromospheric and coronal twisted structures. Moreover, it allows us to map and identify the direct and return currents in the sunspots. Finally, this decomposition of j{sub z} is general and can be applied to any vector magnetogram in order to better identify the weaker large-scale currents that are associated with coronal twisted/sheared structures.},
doi = {10.1088/0004-637X/793/1/15},
journal = {Astrophysical Journal},
issn = {0004-637X},
number = 1,
volume = 793,
place = {United States},
year = {2014},
month = {9}
}