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authorPrashant S2020-04-14 10:25:32 +0530
committerGitHub2020-04-14 10:25:32 +0530
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+{
+"cells": [
+ {
+ "cell_type": "markdown",
+ "metadata": {},
+ "source": [
+ "# Chapter 1: Thermal Radiation and Plancks Postulate"
+ ]
+ },
+{
+ "cell_type": "markdown",
+ "metadata": {},
+ "source": [
+ "## Example 1.1: Surface_temperature_calculatio.sce"
+ ]
+ },
+ {
+"cell_type": "code",
+ "execution_count": null,
+ "metadata": {
+ "collapsed": true
+ },
+ "outputs": [],
+"source": [
+"//Example 1.1, page 24\n",
+"clear\n",
+"//For sun\n",
+"sigma=5.67*10^-8//w/m^2-k^4\n",
+"T=5700//in K\n",
+"ST_sun=sigma*T^4\n",
+"printf('\n Surface temperature of sun is %e W/m^2.',ST_sun)\n",
+"//For north star\n",
+"T=8300//in K\n",
+"ST_Northstar=sigma*T^4\n",
+"printf('\n Surface temperature of sun is %e W/m^2.',ST_Northstar)"
+ ]
+ }
+,
+{
+ "cell_type": "markdown",
+ "metadata": {},
+ "source": [
+ "## Example 1.6: Continious_or_dis_continious_energy.sce"
+ ]
+ },
+ {
+"cell_type": "code",
+ "execution_count": null,
+ "metadata": {
+ "collapsed": true
+ },
+ "outputs": [],
+"source": [
+"//Example 1.6, apge 39\n",
+"clc\n",
+"g=9.8//in m/s^2, constant\n",
+"l=.1//in m\n",
+"m=0.01//in kg\n",
+"h=6.63*10^-34//Joule-sec\n",
+"theta=0.1//in radians\n",
+"v=(1/(2*%pi)*sqrt(g/l))\n",
+"printf('\n Oscillation frequency of pendulam %f per sec.',v)\n",
+"E=m*g*l*(1-cos(theta))\n",
+"printf('\n Energy of pendulum at its maximum potential %e Joule.',E)\n",
+"Delta_e=h*v\n",
+"printf('\n Delta E %e Joule',Delta_e)"
+ ]
+ }
+],
+"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
+}