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Fix typos #2821

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9 changes: 2 additions & 7 deletions source/postprocess/mass_flux_statistics.cc
Expand Up @@ -72,11 +72,6 @@ namespace aspect
// mass flux and that is owned by this processor,
// integrate the normal mass flux given by the formula
// j = \rho * v * n
//
// for the spherical shell geometry, note that for the inner boundary,
// the normal vector points *into* the core, i.e. we compute the flux
// *out* of the mantle, not into it. we fix this when we add the local
// contribution to the global flux
for (; cell!=endc; ++cell)
if (cell->is_locally_owned())
for (unsigned int f=0; f<GeometryInfo<dim>::faces_per_cell; ++f)
Expand Down Expand Up @@ -130,7 +125,7 @@ namespace aspect
global_boundary_fluxes[*p] = global_values[index];
}

// now add all of the computed heat fluxes to the statistics object
// now add all of the computed mass fluxes to the statistics object
// and create a single string that can be output to the screen
std::ostringstream screen_text;
unsigned int index = 0;
Expand Down Expand Up @@ -186,7 +181,7 @@ namespace aspect
"the core into the mantle when the domain describes the "
"mantle, then you need to multiply the result by -1."
"\n\n"
"\\note{In geodynamics, the term ``mass flux'' is often understand "
"\\note{In geodynamics, the term ``mass flux'' is often understood "
"to be the quantity $\\rho \\mathbf v$, which is really a mass "
"flux \\textit{density}, i.e., a vector-valued field. In contrast "
"to this, the current postprocessor only computes the integrated "
Expand Down