Changes between Version 19 and Version 20 of PlanetaryAtmospheres
- Timestamp:
- 08/31/15 11:54:26 (9 years ago)
Legend:
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PlanetaryAtmospheres
v19 v20 51 51 || $\xi_{Mp}=\frac{\lambda_p}{2} \xi_p$ || Ratio of sonic radius of planetary wind to planetary orbital radius || 52 52 || $\chi_{bow} = \frac{\rho_p \left ( r_{bow} \right )}{\rho_s \left ( a-r_{bow} \right )}$ || Density ratio at bow shock. || 53 || $\xi_{Ms}=\frac{\lambda_ p}{2} \xi_s$ || Ratio of sonic radius of stellar wind to planetary orbital radius ||53 || $\xi_{Ms}=\frac{\lambda_s}{2} \xi_s$ || Ratio of sonic radius of stellar wind to planetary orbital radius || 54 54 || $\sigma_{p,bow} = \frac{B_p^2 R_p^6}{r_{bow} ^6 \rho_p \left( r_{bow} \right ) \left ( c_p^2+v_p \left(r_{bow} \right)^2 \right ) }$ || Ratio of planetary magnetic pressure to ram pressure (plus thermal) at bow shock || 55 55 || $\sigma_{s,bow} = \frac{B_s^2 R_s^6}{\left ( a - r_{bow} \right ) ^6 \rho_s \left( a - r_{bow} \right ) \left ( c_s^2+v_s \left(a - r_{bow} \right)^2 \right ) }$ || Ratio of stellar magnetic pressure to ram pressure (plus thermal) at bow shock ||
