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arXiv · 2008.04179

High-frequency oscillations in small chromospheric bright features observed with ALMA

Juan Camilo Guevara Gómez·Shahin Jafarzadeh·Sven Wedemeyer·Mikolaj Szydlarski·Marco Stangalini·Bernhard Fleck·Peter Keys
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Abstract

We report detection of oscillations in brightness temperature, size, and horizontal velocity of three small bright features in the chromosphere of a plage/enhanced-network region. The observations, which were taken with high temporal resolution (i.e., 2-sec cadence) with the Atacama Large Millimeter/submillimeter Array (ALMA) in Band 3 (centred at 3 mm; 100 GHz), exhibit three small-scale features with oscillatory behaviour with different, but overlapping, distributions of period on the order of, on average, $90 \pm 22$ s, $110 \pm 12$ s and $66 \pm 23$ s, respectively. We find anti-correlations between perturbations in brightness temperature and size of the three features, which suggest the presence of fast sausage-mode waves in these small structures. In addition, the detection of transverse oscillations (although with a larger uncertainty) may suggest as well the presence of Alfvénic oscillations which are likely representative of kink waves. This work demonstrates the diagnostic potential of high-cadence observations with ALMA for detecting high-frequency magnetohydrodynamic waves in the solar chromosphere. Such waves can potentially channel a vast amount of energy into the outer atmosphere of the Sun.

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Juan Camilo Guevara Gómez, Shahin Jafarzadeh, Sven Wedemeyer, Mikolaj Szydlarski, Marco Stangalini, Bernhard Fleck, Peter Keys. 2020-08-10. High-frequency oscillations in small chromospheric bright features observed with ALMA. https://doi.org/10.1098/rsta.2020.0184

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