getting into the hard coding part

module2/exo1/Untitled.ipynb

+{
+ "cells": [],
+ "metadata": {},
+ "nbformat": 4,
+ "nbformat_minor": 4
+}

module2/exo1/toy_notebook_fr.ipynb

@@ -17,7 +17,7 @@
   },
   {
    "cell_type": "code",
-   "execution_count": 4,
+   "execution_count": 14,
    "metadata": {},
    "outputs": [],
    "source": [
@@ -31,7 +31,7 @@
   },
   {
    "cell_type": "code",
-   "execution_count": 5,
+   "execution_count": 15,
    "metadata": {},
    "outputs": [],
    "source": [
@@ -73,6 +73,85 @@
     "    return lines"
    ]
   },
+  {
+   "cell_type": "markdown",
+   "metadata": {},
+   "source": [
+    "## Etude de la dépendance entre le Mshell et la position de l'équateur centrifuge\n",
+    "**Note :** Une partie importante de l'étude a déjà été fait en amont : le calcul, pour un certain échantillonage de l'équateur centrifuge en rayon sphérique $r_{cent}$ et en longitude $\\phi_{cent}$, de la latitude $\\lambda_{cent}$ et du $Mshell$ correspondant. Ces données sont chargées sur ce document computationnel à partir d'un document texte.  "
+   ]
+  },
+  {
+   "cell_type": "markdown",
+   "metadata": {},
+   "source": [
+    "### Tentative de détection de tendances\n",
+    "Dans la suite, je travaille les données directement pour tenter de faire ressortir des tendances $Mshell = f(\\phi_{cent})$ et $Mshell = f(r_{cent})$ à $r_{cent}$ et $\\phi_{cent}$ fixés respectivement.  "
+   ]
+  },
+  {
+   "cell_type": "code",
+   "execution_count": 22,
+   "metadata": {},
+   "outputs": [],
+   "source": [
+    "# parametres utilisateur\n",
+    "model = 'JRM33+CON2020'  # magnetic field model used\n",
+    "npoints = 100, 60\n",
+    "radlims = (\"5\", \"30\")\n",
+    "savefiletitle = \"centrifugalequator_radius{}min{}max{}pts_latitude_longitude{}pts_\"\\\n",
+    "                \"mshell{}\".format(radlims[0], radlims[1], npoints[1], npoints[0], model)"
+   ]
+  },
+  {
+   "cell_type": "code",
+   "execution_count": 23,
+   "metadata": {},
+   "outputs": [
+    {
+     "ename": "FileNotFoundError",
+     "evalue": "[Errno 2] No such file or directory: 'centrifugalequator_radius5min30max60pts_latitude_longitude100pts_mshellJRM33+CON2020.txt'",
+     "output_type": "error",
+     "traceback": [
+      "\u001b[0;31m---------------------------------------------------------------------------\u001b[0m",
+      "\u001b[0;31mFileNotFoundError\u001b[0m                         Traceback (most recent call last)",
+      "\u001b[0;32m<ipython-input-23-a48f043da36a>\u001b[0m in \u001b[0;36m<module>\u001b[0;34m\u001b[0m\n\u001b[1;32m      1\u001b[0m \u001b[0;31m# definition et completion des tableaux de donnees a partir du fichier texte\u001b[0m\u001b[0;34m\u001b[0m\u001b[0;34m\u001b[0m\u001b[0m\n\u001b[1;32m      2\u001b[0m \u001b[0mmshells\u001b[0m \u001b[0;34m,\u001b[0m\u001b[0mradiis\u001b[0m\u001b[0;34m,\u001b[0m \u001b[0mlongitudes\u001b[0m\u001b[0;34m,\u001b[0m\u001b[0mlatitudes\u001b[0m \u001b[0;34m=\u001b[0m \u001b[0mnp\u001b[0m\u001b[0;34m.\u001b[0m\u001b[0mzeros\u001b[0m\u001b[0;34m(\u001b[0m\u001b[0mnpoints\u001b[0m\u001b[0;34m)\u001b[0m\u001b[0;34m,\u001b[0m \u001b[0mnp\u001b[0m\u001b[0;34m.\u001b[0m\u001b[0mzeros\u001b[0m\u001b[0;34m(\u001b[0m\u001b[0mnpoints\u001b[0m\u001b[0;34m)\u001b[0m\u001b[0;34m,\u001b[0m \u001b[0mnp\u001b[0m\u001b[0;34m.\u001b[0m\u001b[0mzeros\u001b[0m\u001b[0;34m(\u001b[0m\u001b[0mnpoints\u001b[0m\u001b[0;34m)\u001b[0m\u001b[0;34m,\u001b[0m \u001b[0mnp\u001b[0m\u001b[0;34m.\u001b[0m\u001b[0mzeros\u001b[0m\u001b[0;34m(\u001b[0m\u001b[0mnpoints\u001b[0m\u001b[0;34m)\u001b[0m\u001b[0;34m\u001b[0m\u001b[0m\n\u001b[0;32m----> 3\u001b[0;31m \u001b[0mlines\u001b[0m \u001b[0;34m=\u001b[0m \u001b[0mextractfilelines\u001b[0m\u001b[0;34m(\u001b[0m\u001b[0msavefiletitle\u001b[0m\u001b[0;34m+\u001b[0m\u001b[0;34m\".txt\"\u001b[0m\u001b[0;34m)\u001b[0m\u001b[0;34m\u001b[0m\u001b[0m\n\u001b[0m\u001b[1;32m      4\u001b[0m \u001b[0mk\u001b[0m \u001b[0;34m=\u001b[0m \u001b[0;36m0\u001b[0m\u001b[0;34m\u001b[0m\u001b[0m\n\u001b[1;32m      5\u001b[0m \u001b[0;32mfor\u001b[0m \u001b[0mi\u001b[0m \u001b[0;32min\u001b[0m \u001b[0mrange\u001b[0m\u001b[0;34m(\u001b[0m\u001b[0mnpoints\u001b[0m\u001b[0;34m[\u001b[0m\u001b[0;36m0\u001b[0m\u001b[0;34m]\u001b[0m\u001b[0;34m)\u001b[0m\u001b[0;34m:\u001b[0m\u001b[0;34m\u001b[0m\u001b[0m\n",
+      "\u001b[0;32m<ipython-input-15-522922b900e5>\u001b[0m in \u001b[0;36mextractfilelines\u001b[0;34m(filename, titlemarker)\u001b[0m\n\u001b[1;32m     26\u001b[0m     \u001b[0;31m# into a list of its lines in text format\u001b[0m\u001b[0;34m\u001b[0m\u001b[0;34m\u001b[0m\u001b[0m\n\u001b[1;32m     27\u001b[0m     \u001b[0;31m# -----------------------------------------------\u001b[0m\u001b[0;34m\u001b[0m\u001b[0;34m\u001b[0m\u001b[0m\n\u001b[0;32m---> 28\u001b[0;31m     \u001b[0;32mwith\u001b[0m \u001b[0mopen\u001b[0m\u001b[0;34m(\u001b[0m\u001b[0mfilename\u001b[0m\u001b[0;34m,\u001b[0m \u001b[0;34m\"r\"\u001b[0m\u001b[0;34m)\u001b[0m \u001b[0;32mas\u001b[0m \u001b[0mf\u001b[0m\u001b[0;34m:\u001b[0m\u001b[0;34m\u001b[0m\u001b[0m\n\u001b[0m\u001b[1;32m     29\u001b[0m         \u001b[0;31m# read title\u001b[0m\u001b[0;34m\u001b[0m\u001b[0;34m\u001b[0m\u001b[0m\n\u001b[1;32m     30\u001b[0m         \u001b[0mline\u001b[0m \u001b[0;34m=\u001b[0m \u001b[0mf\u001b[0m\u001b[0;34m.\u001b[0m\u001b[0mreadline\u001b[0m\u001b[0;34m(\u001b[0m\u001b[0;34m)\u001b[0m\u001b[0;34m\u001b[0m\u001b[0m\n",
+      "\u001b[0;31mFileNotFoundError\u001b[0m: [Errno 2] No such file or directory: 'centrifugalequator_radius5min30max60pts_latitude_longitude100pts_mshellJRM33+CON2020.txt'"
+     ]
+    }
+   ],
+   "source": [
+    "# definition et completion des tableaux de donnees a partir du fichier texte\n",
+    "mshells ,radiis, longitudes,latitudes = np.zeros(npoints), np.zeros(npoints), np.zeros(npoints), np.zeros(npoints)\n",
+    "lines = extractfilelines(savefiletitle+\".txt\")\n",
+    "k = 0\n",
+    "for i in range(npoints[0]):\n",
+    "    for j in range(npoints[1]):\n",
+    "        line = lines[k]\n",
+    "        strvals = line.strip().split()\n",
+    "\n",
+    "        radiis[i, j] = float(strvals[0].strip())\n",
+    "        latitudes[i, j] = float(strvals[1].strip())\n",
+    "        longitudes[i, j] = float(strvals[2].strip())\n",
+    "        mshells[i, j] = float(strvals[3].strip())"
+   ]
+  },
+  {
+   "cell_type": "code",
+   "execution_count": null,
+   "metadata": {},
+   "outputs": [],
+   "source": [
+    "# test du format des tableaux de donnees\n",
+    "for k in range(0, npoints[0], npoints[0]//5):\n",
+    "    print(\"Values on line \"+str(k))\n",
+    "    print(\"r in [{:.2f}, {:.2f}] RJ ; phi in [{:.2f}, {:.2f}] deg ; lambda in [{:.2f}, {:.2f}] deg ; \"\\\n",
+    "          \"mshell in [{:.2f}, {:.2f}] RJ\".format(np.min(radiis[k]), np.max(radiis[k]), np.min(longitudes[k]), \n",
+    "                                                 np.max(longitudes[k]), np.min(latitudes[k]), np.max(latitudes[k]), \n",
+    "                                                 np.min(mshells[k]), np.max(mshells[k])))"
+   ]
+  },
   {
    "cell_type": "code",
    "execution_count": null,