The counterkink rotation of a non-hale active region
We describe the long-term evolution of a bipolar non-Hale active region that was observed from 1995 October to 1996 January. During these four solar rotations the sunspots and subsequent flux concentrations, during the decay phase of the region, were observed to move in such a way that by December t...
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2000
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| Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_0004637X_v544_n1PART1_p540_LopezFuentes http://hdl.handle.net/20.500.12110/paper_0004637X_v544_n1PART1_p540_LopezFuentes |
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