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Earth, Planets and Space
Fig. 6. | Earth, Planets and Space

Fig. 6.

From: Thermal and hydrostatic structure of the protoplanetary disks: Influences of wind strengths, mass distributions, and stellar wind velocity laws

Fig. 6.

The velocity, temperature and height based on Parker’s solution. Panel (a) shows the velocity distribution, (b) the temperature distributions, and (c) the height of the disk for the case of t*/β = 1 × 1012 yr. Subscripts p and c denote the results calculated by Parker’s solution and the constant velocity model in the case of β(r) = 1, respectively.

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