From 158d4b0e369f8ba158b5aaa900f845fa73066f2d Mon Sep 17 00:00:00 2001 From: Michael Zingale Date: Fri, 24 May 2024 10:36:19 -0400 Subject: [PATCH] fix spell from updated codespell (#2854) --- .codespell-ignore-words | 1 + Docs/source/Hydrodynamics.rst | 2 +- Docs/source/Verification.rst | 2 +- Source/hydro/Castro_hydro.H | 10 +++++----- 4 files changed, 8 insertions(+), 7 deletions(-) diff --git a/.codespell-ignore-words b/.codespell-ignore-words index 5a235e1f40..642de727d6 100644 --- a/.codespell-ignore-words +++ b/.codespell-ignore-words @@ -12,3 +12,4 @@ nd ue bion aas +checkin \ No newline at end of file diff --git a/Docs/source/Hydrodynamics.rst b/Docs/source/Hydrodynamics.rst index 9c22cf8fa9..3c76706eda 100644 --- a/Docs/source/Hydrodynamics.rst +++ b/Docs/source/Hydrodynamics.rst @@ -609,7 +609,7 @@ behavior: Compute Primitive Variables --------------------------- -We compute the primtive variables from the conserved variables. +We compute the primitive variables from the conserved variables. - :math:`\rho, \rho e`: directly copy these from the conserved state vector diff --git a/Docs/source/Verification.rst b/Docs/source/Verification.rst index 631cba3ef6..d121821551 100644 --- a/Docs/source/Verification.rst +++ b/Docs/source/Verification.rst @@ -495,7 +495,7 @@ test problem. A hot sphere is centered at the origin in a spherical geometry. The spectrum from this sphere follows a Planck distribution. The ambient medium is at a much lower temperature. A frequency-dependent opacity makes the domain optically thin for high -frequecies and optically thick for low frequency. At long times, the +frequencies and optically thick for low frequency. At long times, the solution will be a combination of the blackbody radiation from the ambient medium plus the radiation that propagated from the hot sphere. An analytic solution exists :cite:`graziani:2008` which gives the diff --git a/Source/hydro/Castro_hydro.H b/Source/hydro/Castro_hydro.H index 776aee48cc..960d83acaf 100644 --- a/Source/hydro/Castro_hydro.H +++ b/Source/hydro/Castro_hydro.H @@ -89,7 +89,7 @@ amrex::Array4 const& srcQ); /// -/// the actual work routine that does the conversion of conserved to primtiive +/// the actual work routine that does the conversion of conserved to primitive /// variables. /// /// @param bx the box to operate over @@ -350,7 +350,7 @@ /// @param idir coordinate direction (0 = x, 1 = y, 2 = z) /// @param q_arr the primitive variable state /// @param flatn_arr flattening coefficient -/// @param dq slope of the primtiive variables +/// @param dq slope of the primitive variables /// @param qm left interface state, e.g., q_{i-1/2,j,k,L} /// @param qp right interface state, e.g., q_{i-1/2,j,k,R} /// @@ -603,7 +603,7 @@ amrex::Real cdtdx_t1, amrex::Real cdtdx_t2); /// -/// Reconstruct the primtive state as parabola, integrate under them, +/// Reconstruct the primitive state as parabola, integrate under them, /// and perform the characteristic tracing to get the interface states. /// This is for the CTU hydrodynamics scheme. /// @@ -634,7 +634,7 @@ const amrex::Real dt); /// -/// Reconstruct the primtive state as pieceeise linear, integrate under them, +/// Reconstruct the primitive state as pieceeise linear, integrate under them, /// and perform the characteristic tracing to get the interface states. /// This is for the CTU hydrodynamics scheme. /// @@ -665,7 +665,7 @@ const amrex::Real dt); /// -/// Reconstruct the primtive state as parabola, integrate under them, +/// Reconstruct the primitive state as parabola, integrate under them, /// and perform the characteristic tracing to get the interface states. /// This is for the CTU radiation hydrodynamics scheme. ///