Heating of chromospheric magnetic featur
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Satoshi Hinata
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Article
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1983
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Springer
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English
โ 392 KB
It is shown that the direct current dissipation is very unlikely to be the heat source of the coronal loop, because it accompanies unacceptably high heating rate in the chromospheric portion of the loop. This also suggests that a rather weak current density can supply the heat to a small (R < 107 cm