Shapefile Components 🔹 .shp — Geometry file What it contains: • The actual geographic shapes (points, lines, polygons) Examples: • City locations (points) • Roads (lines) • Administrative boundaries (polygons) 📌 This is the core file — without it, there is no map. ⸻ 🔹 .shx — Shape index file What it contains: • An index of the geometry file • Allows fast access to shapes 📌 Improves performance when loading and navigating data. ⸻ 🔹 .dbf — Attribute table What it contains: • Attribute data linked to each shape • Stored in dBASE format Examples: • Name, population, area, ID • Road type, length, category 📌 Each row corresponds to one geometry in the .shp file. ⸻ 🔹 .prj — Projection file What it contains: • Coordinate Reference System (CRS) information • Projection, datum, units 📌 Without this file, GIS software does not know where the data is on Earth. ⸻ 🧩 Optional (But Common) Shapefile Files 🔹 .cpg — Character encoding What it contains: • Text encoding for the .dbf file (UTF-8, Latin1, etc.) 📌 Prevents issues with special characters and accents. ⸻ 🔹 .sbn / .sbx — Spatial index files What they contain: • Spatial indexing for faster rendering and queries 📌 Automatically created by some GIS software. ⸻ 🔹 .xml — Metadata file What it contains: • Dataset description • Source, author, creation date, data quality
1. Principles Thermal Infrared Remote Sensing is based on the detection of naturally emitted electromagnetic radiation from objects, rather than reflected solar energy. According to Planck's Radiation Law , all objects with a temperature above absolute zero (0 K) emit electromagnetic radiation. For Earth surface features, the peak emission lies in the Thermal Infrared (TIR) region of 3–14 μm of the electromagnetic spectrum. The amount of radiation emitted is primarily a function of surface temperature and emissivity . Sensors measure the radiant energy flux density (W/m²) , which is later converted to surface temperature using Stefan-Boltzmann's Law . 2. Radiation Properties in TIR Emissivity (ε): Ratio of radiation emitted by a surface to that emitted by a perfect blackbody at the same temperature. Natural surfaces like water (ε ≈ 0.98) have high emissivity, while bare soils and metals have lower values. Blackbody: An idealized object th...
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