Remote sensing, four basic radiation laws help us understand how objects give off and interact with energy (electromagnetic radiation). These laws link an object's temperature , wavelength , and the amount of energy it gives off: 1. Planck's Law Every object that has a temperature (above absolute zero) gives off energy at all wavelengths. But how much it gives off at each wavelength depends on its temperature. This law explains the full energy pattern (spectrum) of a hot object. 2. Stefan-Boltzmann Law Hotter objects give off more total energy. The energy released increases quickly as temperature rises — to the fourth power of the temperature. 3. Wien's Displacement Law Hotter objects give off energy at shorter wavelengths (like blue light), while cooler objects emit at longer wavelengths (like red or infrared). So, the color (or wavelength) of maximum emission shifts based on temperature. 4. Kirchhoff's Law If an object absorbs energy well at a cert...
Remote sensing is the science of collecting information about the Earth from a distance, usually using satellites or aircraft — without touching the surface. Basic Principles of Remote Sensing Energy Source (Sun) ☀️ Everything starts with the Sun , which sends energy (light) to Earth. Interaction with Earth 🌳🏙️💧 This energy hits the Earth's surface — like forests, water, buildings — and gets: Reflected Absorbed Transmitted Sensors Detect the Energy 🛰️ Satellites or aircraft have sensors (cameras) that capture the reflected energy. Data Transmission 📡 The sensors send the collected data back to ground stations . Image Processing 💻 The raw data is processed into images or maps using computer software. Analysis 🧑💼 Scientists or analysts study the images to find out what's happening — like land use, vegetation health, urban growth, disasters, etc. Example: Imagine you're taking a photo of a city from an a...