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Variations of the Galactic Cosmic Rays in the Recent Solar Cycles

  • Authors: Shuai Fu, Xiaoping Zhang, Lingling Zhao, and Yong Li

2021 The Astrophysical Journal Supplement Series 254 37.

  • Provider: AAS Journals

Caption: Figure 7.

The 27 day averaged solar wind/interplanetary parameters from 1996 to 2020. (a) Sunspot number and annual CME rate. (b) Mean solar polar field strength. (c) HCS tilt angle. (d) IMF magnitude B and its root mean square δB. (e) Estimated parallel MFP λ. (f) Solar wind speed (black curve) and dynamic pressure (cyan curve). (g) The 69.4–237.9 MeV nuc−1 GCR oxygen intensity from ACE/CRIS (normalized to the solar minimum P23/24), and the horizontal dashed line represents the normalized GCR intensity equal to 1. The pink-arrow dip in the GCR intensity was caused by CMEs (see Section 3.4 for details).

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