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Déformation du Profil des Raies liées aux Ondes Sonores dans le Cas Solaire
1966
Transactions of the International Astronomical Union
DISCUSSION P. A. Sturrock. (answering a question by E. A. Spiegel). Radiative losses should be taken into account, and the n, T relationship should then ensure that the energy input from acoustic waves is just sufficient to balance radiative loss. Since the energy loss from acoustic waves is very sensitive to M, this should not effect the n-T profile greatly. C. de Jager. If Shockwave dissipation is only important for M > 1, how should one then explain that the temperature in the upper
doi:10.1017/s0251107x00019611
fatcat:jvevd7tb3zhetp6ratlaomxtsy