Rapid Disappearance of Penumbra-Like Features near a Flaring Polarity Inversion Line: The Hinode Observations

<table>The temporal evolution of the PLFs is shown in sequence of G-band and Ca II H images alternatively. The date and time of the image acquisition is shown on the top of each image. The numbers on the axes represent the pixel.</table>

Advances in Astronomy

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Figure 3

Figure 3: Rapid Disappearance of Penumbra-Like Features near a Flaring Polarity Inversion Line: The Hinode Observations 