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Fig. 6.


Left panel: profiles of absolute difference of the excitation temperatures calculated in this work (MUGA) and the MPS-ALI code and right panel: the same, but compared against calculations made by the RATRAN package. The atmospheric inputs correspond to the SSL = 10° conditions (see Fig. 4 for Tex magnitude). Lines of different colours correspond to the transitions as shown in the label in units of GHz.

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