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Active region fine structure observed at 0.08 arcsec resolution
Schlichenmaier, R.,von der Lü,he, O.,Hoch, S.,Soltau, D.,Berkefeld, T.,Schmidt, D.,Schmidt, W.,Denker, C.,Balthasar, H.,Hofmann, A.,Strassmeier, K. G.,Staude, J.,Feller, A.,Lagg, A.,Solanki, S. K. Springer-Verlag 2016 Astronomy and astrophysics Vol.596 No.-
Slipping reconnection in a solar flare observed in high resolution with the GREGOR solar telescope
Sobotka, M.,Dudí,k, J.,Denker, C.,Balthasar, H.,Jurč,á,k, J.,Liu, W.,Berkefeld, T.,Collados Vera, M.,Feller, A.,Hofmann, A.,Kneer, F.,Kuckein, C.,Lagg, A.,Louis, R. E.,von der Lü Springer-Verlag 2016 Astronomy and astrophysics Vol.596 No.-
Three-dimensional structure of a sunspot light bridge
Felipe, T.,Collados, M.,Khomenko, E.,Kuckein, C.,Asensio Ramos, A.,Balthasar, H.,Berkefeld, T.,Denker, C.,Feller, A.,Franz, M.,Hofmann, A.,Joshi, J.,Kiess, C.,Lagg, A.,Nicklas, H.,Orozco Suá,rez EDP Sciences 2016 Astronomy and astrophysics Vol.596 No.-
Magnetic fields of opposite polarity in sunspot penumbrae
Franz, M.,Collados, M.,Bethge, C.,Schlichenmaier, R.,Borrero, J. M.,Schmidt, W.,Lagg, A.,Solanki, S. K.,Berkefeld, T.,Kiess, C.,Rezaei, R.,Schmidt, D.,Sigwarth, M.,Soltau, D.,Volkmer, R.,von der Luhe, EDP Sciences 2016 Astronomy and astrophysics Vol.596 No.-
COMPARISON BETWEEN Mg II<i>k</i>AND Ca II H IMAGES RECORDED BY SUNRISE/SuFI
Danilovic, S.,Hirzberger, J.,Riethmü,ller, T. L.,Solanki, S. K.,Barthol, P.,Berkefeld, T.,Gandorfer, A.,Gizon, L.,Knö,lker, M.,Schmidt, W.,Rodrí,guez, J. Blanco,Iniesta, J. C. Del Toro IOP Publishing 2014 The Astrophysical journal Vol.784 No.1
<P>We present a comparison of high-resolution images of the solar surface taken in the MgII k and Ca II H channels of the Filter Imager on the balloon-borne solar observatory SUNRISE. The Mg and Ca lines are sampled with 0.48 nm and 0.11 nm wide filters, respectively. The two channels show remarkable qualitative and quantitative similarities in the quiet Sun, in an active region plage and during a small flare. However, the Mg filtergrams display 1.4-1.7 times higher intensity contrast and appear more smeared and smoothed in the quiet Sun. In addition, the fibrils in a plage are wider. Although the exposure time is 100 times longer for Mg images, the evidence suggests that these differences cannot be explained only with instrumental effects or the evolution of the solar scene. The differences at least partially arise because of different line-formation heights, the stronger response of Mg k emission peaks to the higher temperatures, and the larger height range sampled by the broad Mg filter used here. This is evidently manifested during the flare when a surge in Mg evolves differently than in Ca.</P>
TRANSVERSE COMPONENT OF THE MAGNETIC FIELD IN THE SOLAR PHOTOSPHERE OBSERVED BY SUNRISE
Danilovic, S.,Beeck, B.,Pietarila, A.,Schü,ssler, M.,Solanki, S. K.,Martí,nez Pillet, V.,Bonet, J. A.,del Toro Iniesta, J. C.,Domingo, V.,Barthol, P.,Berkefeld, T.,Gandorfer, A.,Knö,lker IOP Publishing 2010 ASTROPHYSICAL JOURNAL LETTERS - Vol.723 No.2
Deep probing of the photospheric sunspot penumbra: no evidence of field-free gaps
Borrero, J. M.,Asensio Ramos, A.,Collados, M.,Schlichenmaier, R.,Balthasar, H.,Franz, M.,Rezaei, R.,Kiess, C.,Orozco Suá,rez, D.,Pastor, A.,Berkefeld, T.,von der Lü,he, O.,Schmidt, D.,Schmid Springer-Verlag 2016 Astronomy and astrophysics Vol.596 No.-
SUNRISE/IMaX OBSERVATIONS OF CONVECTIVELY DRIVEN VORTEX FLOWS IN THE SUN
Bonet, J. A.,Má,rquez, I.,Almeida, J. Sá,nchez,Palacios, J.,Pillet, V. Martí,nez,Solanki, S. K.,del Toro Iniesta, J. C.,Domingo, V.,Berkefeld, T.,Schmidt, W.,Gandorfer, A.,Barthol, P IOP Publishing 2010 ASTROPHYSICAL JOURNAL LETTERS - Vol.723 No.2
Upper chromospheric magnetic field of a sunspot penumbra: observations of fine structure
Joshi, J.,Lagg, A.,Solanki, S. K.,Feller, A.,Collados, M.,Orozco Suá,rez, D.,Schlichenmaier, R.,Franz, M.,Balthasar, H.,Denker, C.,Berkefeld, T.,Hofmann, A.,Kiess, C.,Nicklas, H.,Pastor Yabar, A Springer-Verlag 2016 Astronomy and astrophysics Vol.596 No.-