the photosphere has a boiling appearance why

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They produce the auroras on Earth and canĪlso interfere with our communications. ▪ Solar flares are very energetic streams of protons, electrons, and ions Magnetic field lines going from a north to a south magnetic pole. They usually appear near sunspot groups and appear to trace out ▪ Solar prominences are loops of hydrogen gas that rise above the solar Time needed for the Sun's overall magnetic field to become tangled and Largest number of sunspots) is 11 yr and this appears to be related to the The period between sunspot maxima (when there is the Magnetic north pole & the other to the south pole where field lines stretchīetween them. Sunspots usually come in pairs where one sunspot corresponds to the Some of the hot gas rising from the interior to make the sunspots cooler. ▪ Sunspots are dark, cooler regions on the Sun's surface. Activity on the Sun is manifested in several ways: Separation of the line pair is directly proportional to the strength of the magneticĤ. Gas with a strong magnetic field, two lines rather than one will appear. The energy levels in atoms will further divide. On the Sun in the presence of strong magnetic fields (8000 times that on Earth), Which are related to the magnetic fields. The surface of the Sun is not always peaceful, but can undergo periods of activity Occurs in stars with masses similar to and less than that of the Sun.ģ. This type of heat transport is called convection and Of the heat rising from the interior to the surface of the Sun much like a Light & dark structures known as granulation. ▪ The surface of the photosphere has a mottled appearance with a pattern of

Was first detected on the Sun (via its absorption lines) before it was System arising from most of the known elements. ▪ Since this temperature is lower than that of the interior (which isġ6,000,000 K at the core), we have the classic situation described by

▪ It has a characteristic temperature of 5800 K. Temperature is about 2 million degrees K. ▪ The corona is the outermost layer that extends out to several solar radii. ▪ The chromosphere lies above the photosphere. ▪ The photosphere is the layer that we see.

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The photosphere has a boiling appearance why