Fig. 10 from Dynamics of Magnetic Flux Elements in the Solar Photosphere

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Dynamics of Magnetic Flux Elements in the Solar Photosphere

Authors: A. A. van Ballegooijen, P. Nisenson, R. W. Noyes, M. G. Löfdahl, R. F. Stein, Å. Nordlund, and V. Krishnakumar

van Ballegooijen et al. 1998 The Astrophysical Journal 509 435.

Provider: AAS Journals

Caption: Fig. 10.

(a) Horizontal velocity at a height of 1500 km in the chromosphere, as predicted from the potential‐field model for the region shown in Fig. 9. The longest arrows in this plot correspond to 5 km s⁻¹, and the bold arrows show the direction of the field in regions where the horizontal velocity exceeds 5 km s⁻¹. (b) Separatrices between different flux tubes.

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