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+{
+"cells": [
+ {
+ "cell_type": "markdown",
+ "metadata": {},
+ "source": [
+ "# Chapter 17: Chemistry in the atmosphere"
+ ]
+ },
+{
+ "cell_type": "markdown",
+ "metadata": {},
+ "source": [
+ "## Example 17.1: computation_of_wavelength_of_a_photon_from_energy.sce"
+ ]
+ },
+ {
+"cell_type": "code",
+ "execution_count": null,
+ "metadata": {
+ "collapsed": true
+ },
+ "outputs": [],
+"source": [
+"//computation of wavelength of a photon from energy\n",
+"\n",
+"clear;\n",
+"clc;\n",
+"\n",
+"printf('\t Example 17.1\n');\n",
+"\n",
+"E=498.7*10^3/(6.022*10^23);//energy in J/molecule\n",
+"h=6.63*10^-34;//plancks constant, J s\n",
+"v=E/h;//frequency of the photon, s^-1\n",
+"lambda=3*10^8/v;//wavelength in m, since v*lambda=speed of light in vacuum\n",
+"\n",
+"printf('\t the maximum wavelength of the photon which can dissociate an O2 molecule is : %4.0f nm\n',lambda*10^9);\n",
+"\n",
+"//End"
+ ]
+ }
+,
+{
+ "cell_type": "markdown",
+ "metadata": {},
+ "source": [
+ "## Example 17.3: Radioactive_decay_and_half_life.sce"
+ ]
+ },
+ {
+"cell_type": "code",
+ "execution_count": null,
+ "metadata": {
+ "collapsed": true
+ },
+ "outputs": [],
+"source": [
+"//Radioactive decay and half life\n",
+"\n",
+"clear;\n",
+"clc;\n",
+"\n",
+"printf('\t Example 17.3\n');\n",
+"\n",
+"Rninitial=1;//initial mass of Rn, g\n",
+"\n",
+"Rnfinal=Rninitial*0.5^10;//final mass of Rn, g\n",
+"\n",
+"printf('\t the amount of Rn left after 10 half lives is : %4.1f *10^-4 g\n',Rnfinal*10^4);\n",
+"\n",
+"//End"
+ ]
+ }
+],
+"metadata": {
+ "kernelspec": {
+ "display_name": "Scilab",
+ "language": "scilab",
+ "name": "scilab"
+ },
+ "language_info": {
+ "file_extension": ".sce",
+ "help_links": [
+ {
+ "text": "MetaKernel Magics",
+ "url": "https://github.com/calysto/metakernel/blob/master/metakernel/magics/README.md"
+ }
+ ],
+ "mimetype": "text/x-octave",
+ "name": "scilab",
+ "version": "0.7.1"
+ }
+ },
+ "nbformat": 4,
+ "nbformat_minor": 0
+}