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前言1556年,乔治乌·阿格利科拉(Georguis Agricola)在他的《金属学》一书中描述了各种矿石产生的“烟雾颜色”。这可能是关于利用火焰激发金属样品发出的颜色来鉴定物质的最早的记载。事情若是如此,则它标志了火焰光谱学作为分析工具的肇端。此后几百年,在这个领域内的进展非常缓慢。1704年,牛顿观察了光的颜色,研究了光的性质。但是,直到十九世纪,在分析方法和技术上才出现了令人注目的新的发展和改进。正是在这个世纪,发展了现代分析光谱学的一些基本原则。大部份早期的分析方法都利用火焰作激发光源,时至今天,火焰仍是最重要的光源。目
Foreword In 1556, Georguis Agricola described the “smoke color” of various ores in his book Metalography. This may be the earliest account of the use of flame to stimulate the color of metal samples to identify substances. If so, it marks the beginning of flame spectroscopy as an analytical tool. For hundreds of years thereafter, progress has been slow in this area. In 1704, Newton observed the color of light and studied the properties of light. However, it was not until the nineteenth century that noticeable new developments and improvements were made in analytical methods and techniques. It is in this century that some basic principles of modern analytical spectroscopy have been developed. Most of the early methods of analysis used fire as the source of light, and today the flame is still the most important light source. Head