Документ взят из кэша поисковой машины. Адрес
оригинального документа
: http://crydee.sai.msu.ru/physics/therm/
Дата изменения: Sun May 2 18:15:55 2004
Дата индексирования: Mon Oct 1 21:45:49 2012
Кодировка:
Поисковые слова: comet tail
|
Thermodynamics over the Web
Get thermodynamics values for any combination of temperature,
density and hydrogen mass fraction using MHD, OPAL or ISG
equations of state.
Server runs on Dual Celeron 466MHz with 16MB of RAM,
so please be patient.
Currently, allowed ranges are as follows:
Temperature | 3.0 < lg T < 7.5
|
Density function | -2.0 < lg Q < 1.0
|
Hydrogen abundance | 0.2 < X < 0.8
|
Heavy elements abundance | 0.010 < Z < 0.025
|
Q is rho/(T/10^6)**3, i.e. lg Q = lg rho + 18.0 - 3.0 * lg T
Proceed to entering input values
References
- MHD
- Hummer, D.G., Mihalas, D., 1988. Ap.J. 331, 794-814.
- Mihalas, D., Dappen W. and Hummer, D.G., 1988. Ap.J., 331, 815-825.
- Dappen, W., Mihalas, D., Hummer, D.G. and Mihalas, B.W., 1988. Ap.J., 332, 261-270.
- OPAL
- Rogers, F.J., 1994. in IAU Colloq. 147, The Equation of State in
Astrophysics, ed. G.Chabrier & E.L.Schatzman (Cambridge: Cambridge Univ.
Press), 16
- Rogers, F.J., Swenson, F.J., Iglesias, C.A., 1996. Ap.J., 456,
902-908.
Send your comments to Sergey Ayukov