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Article Dans Une Revue The Astrophysical Journal Année : 2009

Current Buildup in Emerging Serpentine Flux Tubes

Résumé

The increase of magnetic flux in the solar atmosphere during active-region formation involves the transport of the magnetic field from the solar convection zone through the lowest layers of the solar atmosphere, through which the plasma beta changes from >1 to

Dates et versions

hal-03730794 , version 1 (20-07-2022)

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Etienne Pariat, Sophie Masson, Guillaume Aulanier. Current Buildup in Emerging Serpentine Flux Tubes. The Astrophysical Journal, 2009, 701, pp.1911-1921. ⟨10.1088/0004-637X/701/2/1911⟩. ⟨hal-03730794⟩
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