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20102022
most citedThree-dimensional structure of a sunspot light bridge

54 citations · 349 across the 16 of their papers we have counts for

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Showing 2016Show all

11 papers · 1 filter

astro-ph.SR2016★ 54 cited

Three-dimensional structure of a sunspot light bridge

T. Felipe, M. Collados, E. Khomenko +26

Active regions are the most prominent manifestations of solar magnetic fields; their generation and dissipation are fundamental problems in solar physics. Light bridges are commonl…

astro-ph.SR2016★ 15 cited

Spectropolarimetric observations of an arch filament system with the GREGOR solar telescope

H. Balthasar, P. Gömöry, S. J. González Manrique +27

Arch filament systems occur in active sunspot groups, where a fibril structure connects areas of opposite magnetic polarity, in contrast to active region filaments that follow the…

astro-ph.SR2016★ 33 cited

Active region fine structure observed at 0.08 arcsec resolution

R. Schlichenmaier, O. von der Lühe, S. Hoch +19

The various mechanisms of magneto-convective energy transport determines the structure of sunspots and active regions. We characterise the appearance of light bridges and other fin…

astro-ph.SR2016★ 23 cited

Upper Chromospheric Magnetic Field of a Sunspot Penumbra: Observations of Fine Structure

J. Joshi, A. Lagg, S. K. Solanki +22

The fine-structure of magnetic field of a sunspot penumbra in the upper chromosphere is to be explored and compared to that in the photosphere. High spatial resolution spectropolar…

astro-ph.SR2016★ 26 cited

Magnetic fields of opposite polarity in sunspot penumbrae

M. Franz, M. Collados, C. Bethge +25

Context. A significant part of the penumbral magnetic field returns below the surface in the very deep photosphere. For lines in the visible, a large portion of this return field c…

astro-ph.SR2016★ 46 cited

Deep probing of the photospheric sunspot penumbra: no evidence for magnetic field-free gaps

J. M. Borrero, A. Asensio Ramos, M. Collados +24

Some models for the topology of the magnetic field in sunspot penumbrae predict the existence of field-free or dynamically weak-field regions in the deep Photosphere. To confirm or…