Remove empty docs

vavrines · Jan 10, 2024 · 29050fb · 29050fb
1 parent 2954813
commit 29050fb
Show file tree

Hide file tree

Showing 4 changed files with 2 additions and 5 deletions.
diff --git a/docs/make.jl b/docs/make.jl
@@ -13,6 +13,7 @@ using Kinetic.KitBase: aap_hs_diffeq!
 using Kinetic.KitBase: plot_line, plot_contour, write_jld
 using Kinetic.KitML.Solaris
 using Kinetic.KitML.Solaris: load_data, save_model
+using Kinetic.KitBase.FiniteMesh
 using Kinetic.KitBase.FiniteMesh: read_mesh, mesh_connectivity_2D, mesh_cell_center, mesh_cell_area_2D
 
 tutorial_page = [

diff --git a/docs/src/kitml1.md b/docs/src/kitml1.md
@@ -50,9 +50,7 @@ It is important for entropy-based modelling, since the minimization principle wo
 
 ```@docs
 Convex
-ICNN
 FastConvex
-FastICNN
 ```
 Besides, we also provide scientific machine learning training interfaces and I/O methods.
 They are consistent with both [Flux.jl](https://github.com/FluxML/Flux.jl) and [DiffEqFlux.jl](https://github.com/SciML/DiffEqFlux.jl) ecosystem.

diff --git a/docs/src/para_cuda.md b/docs/src/para_cuda.md
@@ -5,7 +5,7 @@ Kinetic enables computation on the graphical architecture on the basis of [CUDA.
 It provides the main programming interface for working with NVIDIA CUDA GPUs. 
 It features a user-friendly array abstraction, a compiler for writing CUDA kernels in Julia, and wrappers for various CUDA libraries.
 In the following, we present an illustrative test of kinetic flux vector splitting method to evaluate upwind flux of the Boltzmann equation.
-The test is conducted on a Tesla K80 GPU on [nextjournal.com](nextjournal.com).
+The test is conducted on a Tesla K80 GPU on [nextjournal.com](https://nextjournal.com).
 We first load all the modules, and do a CPU-based computation.
 
 ```julia

diff --git a/docs/src/solver_post.md b/docs/src/solver_post.md
@@ -3,7 +3,5 @@
 The post-process solver handles the simulation data and visualization.
 
 ```@docs
-plot_line
-plot_contour
 write_jld
 ```