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Update 11/15
- Removed extra refinement from MHD simulations and extended boundaries by 0.025 in each direction. Still have subsonic material leaving grid in x-y plane, as well as both subsonic and sub-alfvenic eventually leaving in the z direction. Also, alfven speed is becoming very large in a concentrated area around frame 24 and increasing computation time significantly - not sure if there's anything to do about this.
Definitely going to increase grid size more. Anything else to do about computation time and irregularity of contours?
- WASP-12b simulations appear to have gone extremely well, on the other hand. Ran a test with new parameters for density, bow shock radius, etc.:
\xi_p | 0.036180 | ratio of planet radius to orbital separation |
\xi_s | 0.324198 | ratio of stellar radius to orbital separation |
\xi_H | 0.069149 | ratio of Hill radius to orbital separation (from planet) |
\xi_{bow} | 0.125384 | ratio of bow shock radius to orbital separation (from planet) |
\xi_{Mp} | 0.314214 | ratio of planet sonic radius to orbital separation (from planet) |
\xi_{\Omega} | 0.314214 | ratio of coriolis radius to orbital separation (from planet) |
\chi_{bow} | 87.507134 | ratio of densities at bow shock |
\lambda_s | 19.542018 | stellar lambda |
\lambda_p | 17.369379 | planetary lambda |
Orbital separation | 0.022930 | AU |
Mass of Star | 1.349999 | solar masses |
Mass of Planet | 1.405393 | Jupiter masses |
Radius of Star | 1.599000 | solar radii |
Radius of Planet | 1.736000 | Jupiter radii |
Temperature of Star | 999999.016096 | Kelvin |
Temperature of Planet | 10009.919196 | Kelvin |
Density of Star | 3.211200e-17 | g/cc |
Density of Planet | 3.211200e-15 | g/cc |
Orbital period | 1.090679 | days |
Mass loss from Star | 1.002167e-18 | solar masses per yr |
Mass loss from Planet | 5.460294e+07 | g/s |
Mach number of Stellar wind at shock | 2.050641e-01 | |
Mach number of Planetary wind at shock | 4.368280e-01 | |
predicted bow shock radius in units of lscale | 1.255086e-01 |
Mass loss rates may be a bit low - can increase both densities to get higher, but sims look good:
Still a slight spiral feature in the initial stellar wind, before planet is created, but doesn't seem to persist (may just be Coriolis effects - doesn't appear to originate from stellar surface). Ran 9 full orbits - reaches quasi-steady state after about 3 days:
- Posted: 8 years ago
- Author: adebrech
- Categories: (none)
Attachments (4)
- wasp.gif (16.7 MB) - added by adebrech 8 years ago.
- wasp_test.gif (3.2 MB) - added by adebrech 8 years ago.
- alfven_larger.gif (3.7 MB) - added by adebrech 8 years ago.
- larger.gif (3.6 MB) - added by adebrech 8 years ago.
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