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Preferential Appearance of Hα Moreton Waves along Photospheric Magnetic Network Boundaries

  • Authors: C. H. Zhai, Y. W. Ni, J. H. Guo, P. F. Chen

C. H. Zhai et al 2026 The Astrophysical Journal Letters 1001 .

  • Provider: AAS Journals

Caption: Figure 2.

Spatial relationship between the Moreton wave front at 12:55:47 UT and different proxies of photospheric networks, i.e., the AIA 1600 Å intensity image (panel (a)), the HMI longitudinal magnetic intensity (panel (b)), and the HMI Dopplergram. The Moreton wave front is indicated by the red dots in panels (a) and (b) and black dots in panel (c).

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