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Alfven wave phase-mixing in flows Why over-dense, solar coronal, open magnetic field structures are cool
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School of Physics and Astronomy
Physics and Astronomy
Alfven wave phase-mixing in flows Why over-dense, solar coronal, open magnetic field structures are cool
QMRO Home
School of Physics and Astronomy
Physics and Astronomy
Alfven wave phase-mixing in flows Why over-dense, solar coronal, open magnetic field structures are cool
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