Abstract
We report on a signature of chromospheric downflows in two emerging flux regions detected by time-distance helioseismology analysis. We use both chromospheric intensity oscillation data in the Ca II H line and photospheric Dopplergrams in the Fe I 557.6 nm line obtained by Hinode/SOT for our analyses. By cross-correlating the Ca II oscillation signals, we have detected a travel-time anomaly in the plage regions; outward travel times are shorter than inward travel times by 0.5-1 minute. However, such an anomaly is absent in the Fe I data. These results can be interpreted as evidence of downflows in the lower chromosphere. The downflow speed is estimated to be below 10 km s -1. This result demonstrates a new possibility of studying chromospheric flows by time-distance analysis. © 2009. The American Astronomical Society. All rights reserved..
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Nagashima, K., Sekii, T., Kosovichev, A. G., Zhao, J., & Tarbell, T. D. (2009). Helioseismic signature of chromospheric downflows in acoustic travel-time measurements from Hinode. Astrophysical Journal, 694(2). https://doi.org/10.1088/0004-637X/694/2/L115
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