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Scientific considerations for future spectroscopic measurements from space of activity on the Sun
DOI: 10.1002/2016JA022651 Bibcode: 2016JGRA..12111667H

Holman, Gordon D.

High-resolution UV and X-ray spectroscopy are important to understanding the origin and evolution of magnetic energy release in the solar atmosphere, as well as the subsequent evolution of heated plasma and accelerated particles. Electromagnetic radiation is observed from plasma heated to temperatures ranging from about 10 kK to above 10 MK, from …

2016 Journal of Geophysical Research (Space Physics)
IRIS 16