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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
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Journal of Geophysical Research (Space Physics)
IRIS
16