Abstract
Presents an outline of the main observational results to date, and the future prospects for spectroscopic studies of solar X-ray and UV emission in the Russian (former Soviet Union) space programme. The investigations of solar XUV line spectra carried out at the P.N. Lebedev Physical Institute of the Russian Academy of Sciences are stressed. A short description of the coronal project, which aims to study the complex nature of the Sun, is also given.
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