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arXiv · 1604.02252

Oscillatory Response of the Solar Chromosphere to a Strong Downflow above a Sunspot

Hannah Kwak·Jongchul Chae·Donguk Song·Yeon-Han Kim·Eun-Kyung Lim·Maria S. Madjarska
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Abstract

We report three-minute oscillations in the solar chromosphere driven by a strong downflow event in a sunspot. We used the Fast Imaging Solar Spectrograph of the 1.6 m New Solar Telescope and the Interface Region Imaging Spectrograph (IRIS). The strong downflow event is identified in the chromospheric and transition region lines above the sunspot umbra. After the event, oscillations occur at the same region. The amplitude of the Doppler velocity oscillations is 2 km/s, and gradually decreases with time. In addition, the period of the oscillations gradually increases from 2.7 minutes to 3.3 minutes. In the IRIS 1330 slit-jaw images, we identify a transient brightening near the footpoint of the downflow detected in the Ha+0.5A image. The characteristics of the downflowing material are consistent with those of sunspot plumes. Based on our findings, we suggest that the gravitationally stratified atmosphere came to oscillate with three minute period in response to the impulsive downflow event as was theoretically investigated by Chae & Goode(2015).

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Hannah Kwak, Jongchul Chae, Donguk Song, Yeon-Han Kim, Eun-Kyung Lim, Maria S. Madjarska. 2016-04-08. Oscillatory Response of the Solar Chromosphere to a Strong Downflow above a Sunspot. https://doi.org/10.3847/2041-8205/821/2/l30

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