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作 者:尤建圻[1]
出 处:《天文学进展》1993年第1期3-12,共10页Progress In Astronomy
摘 要:本文概要地介绍了太阳红外观测的特点,困难和检测技术上的飞速发展。同时,对目前太阳红外观测和研究的结果作了全面评述,其中着重讨论红外波区在取得太阳大气各层次信息中的作用,在红外进行太阳宏观电场和高灵敏磁场测量上的优点及其初步结果。文中还展望了90年代太阳红外观测和研究的前景。An overall review on the observations and researches in infrared solar physics is given in this paper. To begin with, we illustrate the peculiarity and difficulty in the infrared solar obseravtions and present a brief discription about the rapid progress in new technology, especially in the infrared detectors. Then the recent results in the infrared observations and studies of the Sun are summarized with the emphasis on the advantages of the solar infrared observations, such as the rich information of the solar atmosphere from the deepest photpsphere up to the corona and the innovative ways to measure the macroscopic electric fields and vector magnetic fields. Finally the paper outlines the prospects for infrared solar physics in the 1990s.
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