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: | \(\frac{\partial{pe}}{\partial{\theta}}\) |