Открытые коды для расчета звездной эволюции и строения звезд. Созданы международной группой астрофизиков.
Вверх
Таблица 1
Колонки в модели звезды (файлы logn.data)
| 1. | zone | 28. |
grada | 55. | he4 |
| 2. |
logT | 29. | free_e | 56. | c12
|
| 3. |
logRho | 30. |
abar | 57. | n14 |
| 4. |
logP | 31. |
ye
| 58. | o16 |
| 5. |
logR | 32. |
abar
log_opacity
| 59. | ne20 |
| 6. |
luminosity | 33. |
eps_nuc |
60. | mg24 |
| 7. |
eps_grav | 34. |
non_nuc_neu |
61. | pp |
| 8. |
signed_log_eps_grav | 35. |
mlt_mixing_length |
62. | cno |
| 9. |
net_energy | 36. |
mlt_mixing_type |
63. | tri_alfa |
| 10. |
signed_log_power | 37. |
gradT_sub_grada |
64. | burn_c |
| 11. |
velocity | 38. |
log_D_mix |
65. | burn_n |
| 12. |
entropy | 39. |
log_conv_vel |
66. | burn_o |
| 13. |
mixing_type | 40. |
conv_vel_div_csound |
67. | burn_ne |
| 14. |
csound | 41. |
log_mlt_D_mix |
68. | burn_na |
| 15. |
v_div_csound | 42. |
pressure_scale_height |
69. | burn_mg |
| 16. |
eta | 43. |
gradT |
70. | burn_si |
| 17. |
mu | 44. |
gradr |
71. | burn_s |
| 18. |
logdq | 45. |
dlnd_dt |
72. | burn_ar
|
| 19. |
dq_ratio | 46. |
dlnT_dt |
73. | burn_ca |
| 20. |
q | 47. |
signed_dlnd |
74. | burn_ti |
| 21. |
radius | 48. |
signed_dlnT |
75. | burn_cr |
| 22. |
temperature | 49. |
mass |
76. | burn_fe |
| 23. |
tau | 50. |
mmid |
77. | c12_c12 |
| 24. |
logtau | 51. |
logxq |
78. | c12_o16 |
| 25. |
pressure | 52. |
logxm |
79. | o16_o16 |
| 26. |
<>pgas_div_ptotal | 53. |
h1 |
80. | pnhe4 |
| 27. |
logPgas | 54. |
he3 |
81. | photo |
ПРИМЕР ЗАДАЧИ ВНУТРЕННЕГО СТРОЕНИЯ