Spherical harmonic coefficients for "Discovery of a wind-driven diamagnetic current system in the Martian magnetosphere"

The following text files tabulate the derived spherical harmonic coefficients and their estimated uncertainties for the figures of Harada et al. (2025): Fig. S1: gauss_lsall_by0_bc0_alt0250.txt Figs. 1, S2, S3: gauss_lsall_byp_bc0_alt0250.txtgauss_lsall_bym_bc0_alt0250.txt Figs. S4, S5: gauss_byp_pdyn0_alt0250.txtgauss_byp_pdyn1_alt0250.txtgauss_bym_pdyn0_alt0250.txtgauss_bym_pdyn1_alt0250.txt Figs. S6, S7, S8:gauss_ls000_by0_bc0_alt0250.txtgauss_ls090_by0_bc0_alt0250.txtgauss_ls180_by0_bc0_alt0250.txtgauss_ls270_by0_bc0_alt0250.txtgauss_ls000_byp_bc0_alt0250.txtgauss_ls090_byp_bc0_alt0250.txtgauss_ls180_byp_bc0_alt0250.txtgauss_ls270_byp_bc0_alt0250.txtgauss_ls000_bym_bc0_alt0250.txtgauss_ls090_bym_bc0_alt0250.txtgauss_ls180_bym_bc0_alt0250.txtgauss_ls270_bym_bc0_alt0250.txt Figs. S9, S10:gauss_lsall_byp_bc1_alt0250.txtgauss_lsall_byp_bc2_alt0250.txtgauss_lsall_bym_bc1_alt0250.txtgauss_lsall_bym_bc2_alt0250.txt