add pngs in docs/tests/attach

quokka-astro · Jan 4, 2024 · 2608236 · 2608236
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diff --git a/docs/tests/attach/hydro_shuosher.png b/docs/tests/attach/hydro_shuosher.png
diff --git a/docs/tests/attach/hydro_sms.png b/docs/tests/attach/hydro_sms.png
diff --git a/docs/tests/attach/radcoupling.png b/docs/tests/attach/radcoupling.png
diff --git a/docs/tests/attach/radcoupling_rsla.png b/docs/tests/attach/radcoupling_rsla.png
diff --git a/docs/tests/attach/radhydro_pulse_density-1.png b/docs/tests/attach/radhydro_pulse_density-1.png
diff --git a/docs/tests/attach/radhydro_pulse_density.png b/docs/tests/attach/radhydro_pulse_density.png
diff --git a/docs/tests/attach/radhydro_pulse_temperature-1.png b/docs/tests/attach/radhydro_pulse_temperature-1.png
diff --git a/docs/tests/attach/radhydro_pulse_temperature.png b/docs/tests/attach/radhydro_pulse_temperature.png
diff --git a/docs/tests/attach/radhydro_pulse_velocity-1.png b/docs/tests/attach/radhydro_pulse_velocity-1.png
diff --git a/docs/tests/attach/radhydro_pulse_velocity.png b/docs/tests/attach/radhydro_pulse_velocity.png
diff --git a/docs/tests/attach/radhydro_uniform_advecting_temperature-nobeta.png b/docs/tests/attach/radhydro_uniform_advecting_temperature-nobeta.png
diff --git a/docs/tests/attach/radhydro_uniform_advecting_temperature.png b/docs/tests/attach/radhydro_uniform_advecting_temperature.png
diff --git a/docs/tests/attach/radhydro_uniform_advecting_velocity-nobeta.png b/docs/tests/attach/radhydro_uniform_advecting_velocity-nobeta.png
diff --git a/docs/tests/attach/radhydro_uniform_advecting_velocity.png b/docs/tests/attach/radhydro_uniform_advecting_velocity.png
diff --git a/docs/tests/attach/radshock_cgs_temperature.png b/docs/tests/attach/radshock_cgs_temperature.png
diff --git a/docs/tests/radhydro_pulse.rst b/docs/tests/radhydro_pulse.rst
@@ -7,8 +7,8 @@ This test demonstrates the code’s ability to deal with the relativistic
 correction source terms that arise from the mixed frame formulation of
 the RHD moment equations, in a fully-coupled RHD problem. The problems
 involve the advection of the a pulse of radiation energy in an optically
-thick (:math:`\tau \gg 1`) gas in both static (:math:`\beta \tau \gg 1`)
-and dynamic (:math:`\beta \tau \ll 1`) diffusion regimes, with a uniform
+thick (:math:`\tau \gg 1`) gas in both static (:math:`\beta \tau \ll 1`)
+and dynamic (:math:`\beta \tau \gg 1`) diffusion regimes, with a uniform
 background flow velocity :cite:`Krumholz_2007`.
 
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