Fig. 13
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Average spectrum of the main line of CCH hfs component 12,2–01,1 (black line) and the satellite line 11,2–01,0 (gray line, the intensity is artificially enlarged by three times for comparison) along the three PV cuts U, M, L. From left to right, the spectra are arranged from northeast to southwest along the cuts. The blue and red dashed lines follow that in Fig. 10.
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