Cosmogenic nuclides are an excellent proxy of reconstructing the past solar activity. These nuclides are produced in the Earth's atmosphere by nuclear cascade initiated by galactic cosmic ray (GCR) particles, which mainly consist of protons and helium nuclei. As the GCR intensity on Earth is modulated by activity of the solar magnetic field, the past production rate of the cosmogenic nuclides reflects the solar activity at that time (e.g., Beer et al., 2012). To reconstruct the variations of past solar activity, researchers measure the cosmogenic nuclides stored in archived samples, such as 14 C in tree rings and 10 Be in polar ice cores (e.g.,