• Solar Filaments as Tracers of Subsurface Processes

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      http://www.ias.ac.in/article/fulltext/joaa/021/03-04/0177-0183

    • Keywords

       

      Solar filaments; solar dynamo; magnetic fields.

    • Abstract

       

      Solar filaments are discussed in terms of two contrasting paradigms. The standard paradigm is that filaments are formed by condensation of coronal plasma into magnetic fields that are twisted or dimpled as a consequence of motions of the fields' sources in the photo-sphere. According to a new paradigm, filaments form in rising, twisted flux ropes and are a necessary intermediate stage in the transfer to interplanetary space of dynamo-generated magnetic flux. It is argued that the accumulation of magnetic helicity in filaments and their coronal surroundings leads to filament eruptions and coronal mass ejections. These ejections relieve the Sun of the flux generated by the dynamo and make way for the flux of the next cycle.

    • Author Affiliations

       

      D. M. Rust1

      1. Applied Physics Laboratoiy, Johns Hopkins University, 11100 Johns Hopkins Road, Laurel, MD 20723, USA.
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