Stellar Models in TOP
This page describes the star models supported by TOP as well as the fields
defined in the model.
Polytropic Model
Fields:
hh: | |
hht: | |
hhz: | |
hhzz: | |
hhzt: | |
lnhht: | |
lambda: | |
alpha: | |
aplat: | |
omega_K: | |
omga: | |
r_t: | |
r_z: | |
r_map: | |
re_t: | |
re_z: | |
re_map: | |
r_zz: | |
r_zt: | |
r_tt: | |
re_zz: | |
re_zt: | |
re_tt: | |
zeta: | |
cost: | |
sint: | |
cott: | |
CESAM Model
Fields:
rhom: | density \(\rho\) |
rhom_z: | \(\frac{\partial{\rho}}{\partial{\zeta}}\) |
rhom_t: | \(\frac{\partial{\rho}}{\partial{\theta}}\) |
pm: | pressure \(p\) |
pm_z: | \(\frac{\partial{p}}{\partial{\zeta}}\) |
pm_t: | \(\frac{\partial{p}}{\partial{\theta}}\) |
Gamma1: | first adiabatic exponent |
NN: | Brunt-Vaisala frequency (not perturbated) |
NNr: | \(\frac{\partial{NN}}{\partial{\zeta}}\) |
NNt: | \(\frac{\partial{NN}}{\partial{\theta}}\) |
pe: | pressure potential |
pe_z: | \(\frac{\partial{pe}}{\partial{\zeta}}\) |
pe_t: | \(\frac{\partial{pe}}{\partial{\theta}}\) |