| 1 | = Magnetic Fields = |
| 2 | |
| 3 | Calculated with Matlab script: |
| 4 | |
| 5 | __Dimensionless Parameters__ |
| 6 | |
| 7 | || $\xi_p$ || 0.013893 || ratio of planet radius to orbital separation || |
| 8 | || $\xi_s$ || 0.117818 || ratio of stellar radius to orbital separation || |
| 9 | || $\xi_H$ || 0.057598 || ratio of Hill radius to orbital separation (from planet) || |
| 10 | || $\xi_{bow}$ || 0.240468 || ratio of bow shock radius to orbital separation (from planet) || |
| 11 | || $\xi_{Mp}$ || 0.074592 || ratio of planet sonic radius to orbital separation (from planet) || |
| 12 | || $\xi_{\Omega}$ || 0.074592 || ratio of coriolis radius to orbital separation (from planet) || |
| 13 | || $\chi_{bow}$ || 22.853798 || ratio of densities at bow shock || |
| 14 | || $\lambda_s$ || 22.088202 || stellar lambda || |
| 15 | || $\lambda_p$ || 10.738334 || planetary lambda || |
| 16 | || $\sigma_p$ || 0.100000 || |
| 17 | || $\sigma_s$ || 0.100000 || |
| 18 | |
| 19 | __Physical Parameters__ |
| 20 | || Orbital separation || 0.047470 || AU || |
| 21 | || Mass of Star || 1.148000 || solar masses || |
| 22 | || Mass of Planet || 0.690396 || Jupiter masses || |
| 23 | || Radius of Star || 1.203000 || solar radii || |
| 24 | || Radius of Planet || 1.380000 || Jupiter radii || |
| 25 | || Temperature of Star || 999999.671375 || Kelvin || |
| 26 | || Temperature of Planet || 10005.732583 || Kelvin || |
| 27 | || Density of Star || 3.211200e-13 || g/cc || |
| 28 | || Density of Planet || 3.211200e-15 || g/cc || |
| 29 | || Orbital period || 3.523762 || days || |
| 30 | || Magnetic field of Star || 0.059783 Gauss || |
| 31 | || Magnetic field of Planet || 0.052956 Gauss || |
| 32 | || Mass loss from Star || 5.680185e-16 || solar masses per yr || |
| 33 | || Mass loss from Planet || 1.000014e+10 || g/s || |
| 34 | || Mach number of Stellar wind at shock || 6.926105e-01 || || |
| 35 | || Mach number of Planetary wind at shock || 1.448805e+00 || || |
| 36 | || lScale for sim || 7.097443e+11 || cm || |
| 37 | || TimeScale || 3.044531e+05 || s || |
| 38 | || rScale || 3.211200e-15 || g/cc || |
| 39 | || Location of planet in units of lscale || 1.000000e+00 || || |
| 40 | || predicted bow shock radius in units of lscale || 2.406060e-01 || || |
| 41 | |
| 42 | Need to figure out how to determine magnetic radii. Also, check calculation of Bram (cs2?). |
| 43 | |