From e4a36ad20608c410e978406287c67f5f7dd6b4bc Mon Sep 17 00:00:00 2001
From: Richard Hitier <hitier.richard@gmail.com>
Date: Wed, 25 Oct 2023 17:33:48 +0200
Subject: [PATCH] Rename Notebook

---
 notebooks/ConvertAmdaToTaoLike.ipynb     | 66 ------------------------------------------------------------------
 notebooks/Convert_Amda_To_Tao_Like.ipynb | 66 ++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++
 2 files changed, 66 insertions(+), 66 deletions(-)
 delete mode 100644 notebooks/ConvertAmdaToTaoLike.ipynb
 create mode 100644 notebooks/Convert_Amda_To_Tao_Like.ipynb

diff --git a/notebooks/ConvertAmdaToTaoLike.ipynb b/notebooks/ConvertAmdaToTaoLike.ipynb
deleted file mode 100644
index ed8001e..0000000
--- a/notebooks/ConvertAmdaToTaoLike.ipynb
+++ /dev/null
@@ -1,66 +0,0 @@
-{
- "cells": [
-  {
-   "cell_type": "markdown",
-   "id": "b742582b-17be-4f87-a154-02f49de1f4d4",
-   "metadata": {},
-   "source": [
-    "# Convert Amda parameters to build dataset as in tao-datasets\n",
-    "\n",
-    "We would like to plot the Solar Orbiter source. But we need some dataset formated as expected, with following parameters:\n",
-    "\n",
-    "    ncdump -h file.nc\n",
-    "    \n",
-    "    float V(Time) ; V:units = \"km/s\" ;\n",
-    "    float B(Time) ; B:units = \"nT\" ;\n",
-    "    float N(Time) ; N:units = \"cm-3\" ;\n",
-    "    float T(Time) ; T:units = \"eV\" ;\n",
-    "    float Delta_angle(Time) ; Delta_angle:units = \"degrees\" ;\n",
-    "    float P_dyn(Time) ; P_dyn:units = \"nPa\" ;\n",
-    "    \n",
-    "\n",
-    "For the solar obiter data set found on amda, this is like:\n",
-    "|Expected parama |Amda Param|\n",
-    "|--- |------|\n",
-    "|V |pas_momgr1_v_rtn|\n",
-    "|B|solo_b_rtn_tot|\n",
-    "|N|pas_momgr_n|\n",
-    "|T|pas_mom_tav|\n",
-    "|Delta_angle|None|\n",
-    "|P_dyn|None|"
-   ]
-  },
-  {
-   "cell_type": "code",
-   "execution_count": 1,
-   "id": "b2ad3c08-2795-4419-b5b2-71e4b579a2ab",
-   "metadata": {},
-   "outputs": [],
-   "source": [
-    "\n",
-    "from speasy import amda"
-   ]
-  }
- ],
- "metadata": {
-  "kernelspec": {
-   "display_name": "Python 3 (ipykernel)",
-   "language": "python",
-   "name": "python3"
-  },
-  "language_info": {
-   "codemirror_mode": {
-    "name": "ipython",
-    "version": 3
-   },
-   "file_extension": ".py",
-   "mimetype": "text/x-python",
-   "name": "python",
-   "nbconvert_exporter": "python",
-   "pygments_lexer": "ipython3",
-   "version": "3.10.12"
-  }
- },
- "nbformat": 4,
- "nbformat_minor": 5
-}
diff --git a/notebooks/Convert_Amda_To_Tao_Like.ipynb b/notebooks/Convert_Amda_To_Tao_Like.ipynb
new file mode 100644
index 0000000..ed8001e
--- /dev/null
+++ b/notebooks/Convert_Amda_To_Tao_Like.ipynb
@@ -0,0 +1,66 @@
+{
+ "cells": [
+  {
+   "cell_type": "markdown",
+   "id": "b742582b-17be-4f87-a154-02f49de1f4d4",
+   "metadata": {},
+   "source": [
+    "# Convert Amda parameters to build dataset as in tao-datasets\n",
+    "\n",
+    "We would like to plot the Solar Orbiter source. But we need some dataset formated as expected, with following parameters:\n",
+    "\n",
+    "    ncdump -h file.nc\n",
+    "    \n",
+    "    float V(Time) ; V:units = \"km/s\" ;\n",
+    "    float B(Time) ; B:units = \"nT\" ;\n",
+    "    float N(Time) ; N:units = \"cm-3\" ;\n",
+    "    float T(Time) ; T:units = \"eV\" ;\n",
+    "    float Delta_angle(Time) ; Delta_angle:units = \"degrees\" ;\n",
+    "    float P_dyn(Time) ; P_dyn:units = \"nPa\" ;\n",
+    "    \n",
+    "\n",
+    "For the solar obiter data set found on amda, this is like:\n",
+    "|Expected parama |Amda Param|\n",
+    "|--- |------|\n",
+    "|V |pas_momgr1_v_rtn|\n",
+    "|B|solo_b_rtn_tot|\n",
+    "|N|pas_momgr_n|\n",
+    "|T|pas_mom_tav|\n",
+    "|Delta_angle|None|\n",
+    "|P_dyn|None|"
+   ]
+  },
+  {
+   "cell_type": "code",
+   "execution_count": 1,
+   "id": "b2ad3c08-2795-4419-b5b2-71e4b579a2ab",
+   "metadata": {},
+   "outputs": [],
+   "source": [
+    "\n",
+    "from speasy import amda"
+   ]
+  }
+ ],
+ "metadata": {
+  "kernelspec": {
+   "display_name": "Python 3 (ipykernel)",
+   "language": "python",
+   "name": "python3"
+  },
+  "language_info": {
+   "codemirror_mode": {
+    "name": "ipython",
+    "version": 3
+   },
+   "file_extension": ".py",
+   "mimetype": "text/x-python",
+   "name": "python",
+   "nbconvert_exporter": "python",
+   "pygments_lexer": "ipython3",
+   "version": "3.10.12"
+  }
+ },
+ "nbformat": 4,
+ "nbformat_minor": 5
+}
--
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