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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 11.

Upward energy fluxes and the mass fluxes from the chromosphere to the corona in the higher resolution case. The energy fluxes carried by Alfvén (FA) waves, fast-mode waves (Ffast), and slow-mode waves (Fslow) (A)–(D) and the mass flux (E)–(H) varying with time at Y = 1, 5, 12, and 18 Mm are presented.

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