124 | | Note that the vector equation for the numerical flux makes up 3 equations for the 3D Euler equations, one for each component of the following vectors, |
125 | | |
126 | | {{{#!Latex |
127 | | \vec{F}_{i+1/2} = <\rho_{i+1/2}, ~u_{i+1/2}, ~p_{i+1/2}> |
128 | | }}} |
129 | | |
130 | | {{{#!Latex |
131 | | \vec{F}_L = <\rho_L, ~\rho_L * u_L, ~0.5\rho_L*u_L^2 + \frac{p_L}{\gamma - 1}> |
132 | | }}} |
| 124 | Note that the vector equation for the numerical flux makes up 3 equations for the 3D Euler equations, one for each component of the following vectors: the vector of numerical fluxes in conserved form, |
| 125 | {{{#!Latex |
| 126 | \vec{F}_{i+1/2} = <\rho_{i+1/2}, ~p_{i+1/2}, ~E_{i+1/2}> |
| 127 | }}} |
| 128 | |
| 129 | vector of left-fluxes in conserved form, |
| 130 | {{{#!Latex |
| 131 | \vec{F}_L = <\rho_L, ~\rho_L u_L, ~0.5\rho_L u_L^2 + \frac{p_L}{\gamma - 1}> |
| 132 | }}} |
| 133 | |
| 134 | vector of right-fluxes in conserved form, |
| 135 | {{{#!Latex |
| 136 | \vec{F}_L = <\rho_R, ~\rho_R u_R, ~0.5\rho_R u_R^2 + \frac{p_R}{\gamma - 1}> |
| 137 | }}} |
| 138 | |
| 139 | and eigenvectors, |