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The Recent Anomalously Weak Polar Field Does Not Imply a Weak Field at Solar Cycle 25 Minimum

  • Authors: Zi-Fan Wang, Jie Jiang, Yukun Luo, Ruihui Wang, Xinchun Ma, Jing-Xiu Wang

Zi-Fan Wang et al 2026 The Astrophysical Journal Letters 1006 .

  • Provider: AAS Journals

Caption: Figure 4.

Stack plot displaying ARs during CRs 2275–2285. Each tile is obtained from the synoptic maps for photospheric radial magnetic field of HMI, containing only latitudes from 0 to 40 in the northern hemisphere, stacked from the top to bottom in chronological order. White and black indicate positive and negative fields, respectively, and the colors saturate at 100 G. ARs from the database of R. Wang et al. (2023, 2024) are shown by contours. Orange contours mark ARs with unsigned flux less than 4 × 1022 Mx, while green contours mark ARs with unsigned flux greater than 4 × 1022 Mx.

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