EVERY 11 years or so, a new
sunspot
cycle begins. Sunspots are apparent
blemishes
in the sun’s photosphere, the layer which emits its light. Though still hot (about 3,500°C), they are cooler than their surroundings (about 5,500°C) and thus appear dark by contrast. A cycle starts with spots appearing at mid-latitudes in both northern and southern
hemispheres
. Over time, the spot-generating areas migrate towards the equator. As they do so, the amount of light and other radiation the sun emits first increases to a maximum and then decreases to a minimum, until the spots vanish and the cycle renews.
每隔11年左右,太阳黑子就会迎来一个新的活动周期。太阳黑子是太阳光球层(译者注:即太阳向外发射能量的主要大气层)上的明显黑斑,虽然其温度很高,可达到3500°C左右,但与大约5500°C的周围环境相比温度要低得多,所以显得更暗。在活动周期开始时,黑子出现在太阳南北半球的中纬度上。随着时间推移,太阳发出的光能与其它辐射能逐渐达到峰值,随后不断减弱,直至黑子消失,宣告一个完整的黑子活动周期结束。