ISSN:
1476-4687
Source:
Nature Archives 1869 - 2009
Topics:
Biology
,
Chemistry and Pharmacology
,
Medicine
,
Natural Sciences in General
,
Physics
Notes:
[Auszug] For an optically thin plasma in thermodynamic oequilibrium, spectral line intensities can be calculated using the Saha and Boltzmann equations. However, these equations do not hold in the high-temperature plasma produced for thermonuclear research or in the solar corona, and the intensities of ...
Type of Medium:
Electronic Resource
URL:
http://dx.doi.org/10.1038/1981291c0
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