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What Causes the High Apparent Speeds in Chromospheric and Transition Region Spicules on the Sun?

  • Authors: Bart De Pontieu, Juan Martínez-Sykora, and Georgios Chintzoglou

2017 The Astrophysical Journal Letters 849 L7.

  • Provider: AAS Journals

Caption: Figure 4.

Maps of Joule heating due to the ambipolar diffusion (top row), and current density (bottom row) from our numerical simulation reveal currents being propagated at Alfvénic speed and dissipated along already existing spicules. The interval between the snapshots is only 10 s. The temperature at 104 K is shown with white contours.

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