Fig. 3.
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Plasma density and magnetic field profiles obtained by the first fitting step: (A) Plasma density vs. height in Aschwanden’s model of the solar atmosphere. (B) Magnetic field vs. height in three models of the 1 August 2010 zebra with the gyro-harmonic numbers s = 26–30 (full line), s = 10–14 (dotted line), and s = 120–124 (dashed line).
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