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Source: Wikipedia
The Fascinating World of Optical Spectra
Understanding Optical Spectra
The optical spectrum of a light source or beam provides valuable information about how optical energy is distributed across different wavelengths. It is typically represented graphically, showing a spectral quantity plotted against wavelength or optical frequency. This quantity could be spectral flux, spectral intensity, or spectral radiance. Optical spectra can be presented on linear or logarithmic scales, with units such as W/Hz, W/nm, W sr−1 Hz−1, or W sr−1 nm−1.
Characteristics of Optical Spectra
Different light sources exhibit diverse optical spectra. For instance, a supercontinuum source generates a broad spectrum, while a single-frequency laser produces a narrow spectral line. Laser spectra can range from single lines to complex structures like frequency combs in mode-locked lasers for ultrashort pulses.
Optical Bandwidth
The optical bandwidth refers to the width of an optical spectrum and is often defined as the full width at half maximum (FWHM). It provides insights into the range of wavelengths present in the light source.
Optical Spectra with Line Structures
Some light sources have smooth spectra, while others exhibit line structures. For example, continuous-wave lasers with multimode emission may have equidistant lines corresponding to resonator modes. In contrast, mode-locked lasers produce frequency comb spectra with precisely equidistant lines.
Measuring Optical Spectra
Optical spectra are captured using instruments like optical spectrum analyzers, which can be spectrographs or other devices based on interferometric principles. Spectral analysis can also be combined with imaging techniques like multispectral and hyperspectral imaging for comprehensive data collection.
By studying optical spectra, researchers and engineers gain valuable insights into the characteristics and behavior of light sources, enabling advancements in various fields such as telecommunications, spectroscopy, and imaging.
Source: ThoughtCo
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