Sunspots
Error
Sunspot near the limb
Swedish 1m Solar Telescope
This image shows a sunspot near the solar limb as observed through a continuum filter at 436.5 nm. Because of projection effects, granules appear elongated in the direction parallel to the limb and shorter perpendicular to it (the limb is to the left of the image).
Bright small-scale features can be observed on the right side of some granules (i.e., on the side away from the limb). They are called faculae and harbor intense magnetic fields. The gas in their interior is less dense than in the surroundings, so they are more transparent. As a consequence, they allow to see the hot walls of the granule that lie behind them, appearing bright.
The observations were reconstructed using a phase diversity technique.
Image credit: Vasily Zakharov (MPS)
Text credit: Luis Bellot Rubio (IAA-CSIC)
Source: SST Gallery
Regular sunspot observed with CHROMIS
A hole in the Sun (1/2)
A hole in the Sun (2/2)
Sunspot at high spatial resolution (1/3)
Sunspot at high spatial resolution (2/3)
Sunspot at high spatial resolution (3/3)
Sunspot in AR 11302
Sunspot with the Earth shown to scale
Circular polarisation in a sunspot
Sunspot near the limb
Sunspot near the limb
Sunspot and C5-flare
Sunspots, pores, and abnormal granules
[MOVIE] Short-term evolution of sunspots
[MOVIE] Birth of an active region
[MOVIE] Birth and death of an active region
Flux emergence and cancellation in the super-flaring active region 12673 (1/2)
[MOVIE] Flux emergence and cancellation in the super-flaring active region 12673 (2/2)