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Fig. 1

image

Details of the coronal hole model. Initial profiles at the y = 0 plane are shown. Panel a: plasma number density measured in 108 cm−3 (solid line) and magnetic field in G (dashed); panel b: characteristic speeds in the plasma in km s−1, sound speed (solid line) and Alfvén speed (dashed), and magnetoacoustic (MAC) speed in the transverse direction (dotted); and panel c: plasma β* values. See the exact values of parameters of the model in the text.

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