Fig. 12.

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Radial velocity at r = 2 R⊙ for two different simulations where the photospheric density is varied. Panel a: radial velocity taken at t = 40.6 min for the simulation previously described where ρph = 2 × 10−16 g cm3. Panel b: radial velocity from a second simulation at the later time of t = 112.5 min, where the photospheric density has increased by an order magnitude ρph = 2 × 10−15 g cm3. The red circle represents the solar disk which is visible at Earth. Red (blue) corresponds to positive (negative) velocities which are saturated at ±1000 km s−1.
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