(17) A continuous flow of energy is supplied to the photosphere to make good the prodigious losses by radiation. ![]() (16) A continuous flow of energy is supplied to the photosphere to make good the prodigious losses by radiation. (15) The brightness of the photosphere prevents people from seeing the outer layer of the sun's atmosphere. (14) The brightness of the photosphere prevents people from seeing the outer layer of the sun's atmosphere. (13) Detailed studies on magnetic field topology above photosphere have been done. (12) Some people investigate magnetic topology by analyzing magnetic field of photosphere directly. (11) Some people investigate magnetic topology by analyzing magnetic field of photosphere directly. (10) The photosphere is the lowest layer of the sun's atmosphere, and emits the light we see. (9) The photosphere is the lowest layer of the sun's atmosphere, and emits the light we see. (8) From about 200 km above the photosphere outward extension of the height of 100 km area. ![]() (7) From about 20km above the photosphere outward extension of the height of 10km area. (6) Detailed studies on magnetic field topology above photosphere have been done. (5) The chromosphere is a frothy layer churned up by gases in the photosphere. (4) The chromosphere is a frothy layer churned up by gases in the photosphere. (3) The penumbra is the transition from the photosphere to the umbra. (2) The photosphere has a granular structure. ![]() (1) The photosphere has a granular structure.
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