Observations of rotating sunspots and their effect in the corona

Physics

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Sunspots: Rotation, Solar Corona

Scientific paper

Recent observations from TRACE have seen sunspots, in the photospheric white light filter, rotate up to 180 degrees about their umbral centre. The corresponding loops in the coronal fan are seen to twist and can erupt. In an ongoing study, five cases of rotating sunspots have been identified, three of which can be identified with sigmoid structures appearing in Yohkoh/SXT. This paper will present images from one of these events, showing the coupling between the photosphere and the corona, and observational analysis deducing the rotation speeds and how they change through time and with radius of the sunspot. In particular, the paper will focus on the best example of a rotating sunspot observed so far, that of AR 9114 which occurred over 8-10 August 2000 and was observed by TRACE, SoHO/MDI and Yohkoh/SXT. The sunspot rotated 150 degrees within this time and is associated with a sigmoid.

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