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Energy and Mass Transport Associated with Impulsive Spicular Flows in Solar Coronal Holes

  • Authors: Lei Ni, Jun Lin, Tanmoy Samanta, Guanchong Cheng, Yifu Wang, Robert Erdélyi

Lei Ni et al 2026 The Astrophysical Journal Letters 1000 .

  • Provider: AAS Journals

Caption: Figure 8.

Evolutions of the energy density change rate contributed by three different physical effects within a cycle of spicule formation in the 2.5D run with B0 = 5 G. Distributions of the Joule heating (﹩\eta {J}_{z}^{2}﹩) (A–E), compression heating (−P ∇ · V) (F–J), and heat conduction (− ∇ · FC) (K–O) are presented.

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