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Eruptions and jets in the Sun

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Figure

Figure 1.1: (a) The overview of Sun’s structure. (Image credit: http://www.nasa.gov/mission_pages/sunearth/spaceweather/index.html) (b) The Sun’s interior lay-ers
Figure 1.4: Image showing sunspots of different magnetic configurations. (a) A sunspot with a βwork Group (GONG)
Figure 1.5: Image showing a prominence/filament. When observed over the solar limb, it is calleda prominence; when observed on the solar disk, it is called a filament
Figure 4.9: Side (a) and top (b) view of the magnetic field line topology of the first eruption att = 282.81 min.
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