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Global evaluation of coronal heating due to magnetic reconnection based on solar dynamics observatory observations
2015
Radiation effects and defects in solids (Print)
Preserved Fulltext
The explanation to the problem of how the solar corona is heated to the one million degrees temperature has rested on two possible mechanisms; AlfvÃl'n waves traveling upwards from the
doi:10.1080/10420150.2014.993636
fatcat:26mlfmepnvg4vngpi3pw7ym4ge