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Fig. 9

image

Derived LOS magnetic field strength calculated from one half of the simulated FI and FV spectra of the reference circumstellar disk model with different inclinations (113.144 GHz CN line emission). For comparison, a sine function is plotted to show the ideal behavior of the magnetic field component in the LOS direction with inclination. The three roman numerals highlight regions whose LOS magnetic field strengths show different behavior.

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