Thermodynamics of the Convection Zone Through Adiabatic Exponent

Details Thermodynamics of the Convection Zone Through Adiabatic Exponent Thermodynamics of the Convection Zone Through Adiabatic Exponent

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aipc..731..162b&link_type=abstract

EQUATION-OF-STATE AND PHASE-TRANSITION ISSUES IN MODELS OF ORDINARY ASTROPHYSICAL MATTER. AIP Conference Proceedings, Volume 73

Statistics

Applications

Thermodynamic Processes, Conduction, Convection, Equations Of State, Helioseismology, Pulsations, And Shock Waves, Magnetohydrodynamics And Plasmas

Scientific paper

Methods of comparison of the plasma equations of state (EOS) in solar conditions are discussed. The most useful quantity in helioseismic applications is the adiabatic exponent, and its profile is investigated, involving geometric illustration in natural variables - pressure and density. The amount of information which can be obtained about EOS from a profile of adiabatic exponent on an adiabatic curve is studied. The comparison of modern versions of EOS is presented from the point of view of adiabatic profiles.

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