Evidence for Fine Structure in the Chromospheric Umbral Oscillation
Novel spectropolarimetric observations of the He I multiplet are used to explore the dynamics of the chromospheric oscillation above sunspot umbrae. The results presented here provide strong evidence in support of the two-component model proposed by Socas-Navarro and coauthors. According to this model, the waves propagate only inside channels of
Centeno, R. et al.
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12
2005