Fig. 5.
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Height–time diagram (full line) of the radial motion of a fast magnetosonic wave according to Eq. (9) by adopting vA, S = 219 km s−1 and a coronal temperature of 1.39 MK (i.e., λ = 9.88). The crosses show the radial motion of the dome-shaped EUV wave from measurements according to Fig. 2. Here, t = 0 corresponds to 03:50:18 UT in Fig. 2.
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