Эксперимент MIPAS (интерферометр Майкельсона для пассивного зондирования атмосферы) проводился со спутника ENVISAT с использованием Фурье-спектрометра с целью получения инфракрасных лимбовых спектров атмосферы Земли из космоса с высоким разрешением. Возможности измерительной аппаратуры позволяли регистрировать вертикальные профили малых атмосферных газов каждые 75 с как днем, так и ночью с почти полным покрытием всего земного шара. Таким образом получались трехмерные картины состава атмосферы. Для обработки большого потока данных международной группой ученых в рамках контракта ESA была разработана оптимизированная программа потокового анализа данных MIPAS. В постоянном автоматическом режиме данная программа выдает вертикальные профили температуры и давления, а также концентраций таких газов, как O3, H2O, CH4, HNO3, N2O и NO2, для высот от 6 до 68 км. Для анализа и интерпретации лимбовых спектров требуется знание молекулярных параметров этих газов, а также мешающих газов. В данной статье описывается база данных параметров спектральных линий для эксперимента MIPAS.
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