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Multilayered Kelvin–Helmholtz Instability in the Solar Corona
2019 The Astrophysical Journal Letters 884 L51.
Caption: Figure 3.
(a) Position of the plasma blob traced in Figure 2. (b) Average emission intensity in the AIA 193 Å channel and the EM. The time stamps correspond to those labeled in Figure 2.
© 2019. The American Astronomical Society. All rights reserved.
