The Solar Wind.pdf
The Solar Wind.pdf
The Solar Wind.pdf
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• Solvingρ ⎛> ⎜ρ ⎝0r0r⎞⎟⎠1γ −1Where ρ is the density at the base of the atmosphere r 0 .0• From the conservation of mass we getρ ⎛ r< ⎜ρ ⎝ r• <strong>The</strong>se two conditions cannot be solved for3and thereforethe lower atmosphere can’t be adiabatic.• Heat must be supplied from the cooler stellar surface!00⎞⎟⎠2γ =5