Temperature and emission diagnostics of the solar corona : mapping plasma characteristics using multi-channel Extreme UltraViolet observations
The solar corona is a hot, magnetised plasma of which several important aspects remain poorly understood. The Atmospheric Imaging Assembly (AIA) provides very high resolution images of the Sun in several extreme ultraviolet channels. AIA offers a unique chance to improve our understanding of the cor...
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Aberystwyth University
2016
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| Online Access: | https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.690622 |