Fig. 48.
![G-band observations from SOT a few days prior to the 2006 December 13 eruption. The image is overlaid with arrows representing the vector magnetic field. [Reproduced from Magara and Tsuneta (2008).] (Color online)](https://oup.silverchair-cdn.com/oup/backfile/Content_public/Journal/pasj/71/5/10.1093_pasj_psz084/2/pasj_71_5_r1_f43.jpeg?Expires=1749903016&Signature=WoMpd8C3SzQH1njTF1Pr~eJgXT1IrGFuOPAIHQVGLYgnoskJT97jfX8nBxEdAsO64MRTucEmIzpxhIQdcSd5Wz2nwxiiVssRSrl5EQbqOtU0ICw6y0nDP8xFyqoQTAce1OQP2whkVM2zlkEapFedpBWxt00l7f6cgVYGHbZVS4PxtYUDCjMzExNGyyxzLdq07-Yx2CQ5I-wi9juNW78IIzphEM0lYJxqDtLewEE4Rbnm81jIj1ElqFhvoNL53RVzPEXRnwCemdpcdTzHHHtf2XnCH9wJaxTcB11v6DqcZmuKuyvg5d75xS4okr6-iisutUTeley7oU2hpdiH~j2iLg__&Key-Pair-Id=APKAIE5G5CRDK6RD3PGA)
G-band observations from SOT a few days prior to the 2006 December 13 eruption. The image is overlaid with arrows representing the vector magnetic field. [Reproduced from Magara and Tsuneta (2008).] (Color online)
G-band observations from SOT a few days prior to the 2006 December 13 eruption. The image is overlaid with arrows representing the vector magnetic field. [Reproduced from Magara and Tsuneta (2008).] (Color online)
