A Tale of Two Emergences: SUNRISE II Observations of Emergence Sites in a Solar Active Region

被引:31
|
作者
Centeno, R. [1 ]
Blanco Rodriguez, J. [2 ]
Del Toro Iniesta, J. C. [3 ]
Solanki, S. K. [4 ,5 ]
Barthol, P. [4 ]
Gandorfer, A. [4 ]
Gizon, L. [4 ,6 ]
Hirzberger, J. [4 ]
Riethmueler, T. L. [4 ]
van Noort, M. [4 ]
Orozco Suarez, D.
Berkefeld, T. [7 ]
Schmidt, W. [7 ]
Pillet, V. Martinez [8 ]
Knoelker, M. [1 ]
机构
[1] Natl Ctr Atmospher Res, High Altitude Observ, POB 3000, Boulder, CO 80307 USA
[2] Univ Valencia, Grp Astron & Ciencias Espacio, E-46980 Valencia, Spain
[3] CSIC, Inst Astrofis Andalucia, Apartado Correos 3004, E-18080 Granada, Spain
[4] Max Planck Inst Sonnensyst Forsch, Justus von Liebig Weg 3, D-37077 Gottingen, Germany
[5] Kyung Hee Univ, Sch Space Res, Yongin 446701, Gyeonggi, South Korea
[6] Georg August Univ Gottingen, Inst Astrophys, Friedrich Hund Pl 1, D-37077 Gottingen, Germany
[7] Kiepenheuer Inst Sonnenphys, Schoneckstr 6, D-79104 Freiburg, Germany
[8] Natl Solar Observ, 3665 Discovery Dr, Boulder, CO 80303 USA
来源
基金
新加坡国家研究基金会; 美国国家科学基金会;
关键词
Sun: chromosphere; Sun: magnetic fields; Sun: photosphere; sunspots; techniques: polarimetric; SIZED MAGNETIC-BUBBLES; FLUX TUBE EMERGENCE; CONVECTION ZONE; GRANULATION; INSTRUMENT; INVERSION; DYNAMICS; ORIGIN;
D O I
10.3847/1538-4365/229/1/3
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In 2013 June, the two scientific instruments on. board the second SUNRISE mission witnessed, in detail, a small-scale magnetic flux emergence event as part of the birth of an active region. The Imaging Magnetograph Experiment (IMaX) recorded two small (similar to 5 '') emerging flux patches in the polarized filtergrams of a photospheric Fe I spectral line. Meanwhile, the SUNRISE Filter Imager (SuFI) captured the highly dynamic chromospheric response to the magnetic fields pushing their way through the lower solar atmosphere. The serendipitous capture of this event offers a closer look at the inner workings of active region emergence sites. In particular, it reveals in meticulous detail how the rising magnetic fields interact with the granulation as they push through the Sun's surface, dragging photospheric plasma in their upward travel. The plasma that is burdening the rising field slides along the field lines, creating fast downflowing channels at the footpoints. The weight of this material anchors this field to the surface at semi-regular spatial intervals, shaping it in an undulatory fashion. Finally, magnetic reconnection enables the field to release itself from its photospheric anchors, allowing it to continue its voyage up to higher layers. This process releases energy that lights up the arch-filament systems and heats the surrounding chromosphere.
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页数:12
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