The "optical" surface of the Sun (known as the photosphere) is known to have a temperature of approximately 6,000 K.
Above it lies the solar corona, rising to a temperature of around 1,000,000-2,000,000 K The temperature of the photosphere is 6,000 k.
Sunspots are temporary dark spots on the Sun's surface caused by magnetic activity that inhibits the flow of heat. They are cooler and appear darker than the surrounding area of the Sun, indicating intense magnetic activity. Sunspots can vary in size and shape and typically last for a few days to a few weeks.
There is a solar phenomenon believed to be affected by an increase in sunspots. Most solar flares are believed to be linked to an increase in sunspots.
The circulation of gases in the Sun, along with its rotation, creates magnetic fields. These magnetic fields are responsible for various phenomena such as sunspots, solar flares, and the solar wind.
Sunspots are parts of the Sun that are about 1200 degrees centigrade cooler than the surroundings.
Sunspots are regions of cooler gas; however, they are still extremely hot.
Sunspots sit on the sun's photosphere. The photosphere is the surface of the sun, and sunspots are dark regions on it that are visible. The photosphere's average temperature is about 5800 degrees Kelvin.
sunspots
Sunspots
it is the sunspots and thr sun is really really hot
Sun spots and prominences.
Sunspots are temporary dark spots on the Sun's surface caused by magnetic activity that inhibits the flow of heat. They are cooler and appear darker than the surrounding area of the Sun, indicating intense magnetic activity. Sunspots can vary in size and shape and typically last for a few days to a few weeks.
Sunspots on the sun's surface are not directly related to the sun's magnesium content. Sunspots are areas of magnetic activity that appear darker because they are cooler than the surrounding surface. The magnesium content of the sun is relatively stable and does not directly cause the formation of sunspots.
Photosphere- outer (gaseous) layer or surface of sun that we see Faculae- bright areas Sunspots- dark areas
Sunspots are cooler regions on the surface of the sun. Visually, they look like dark circles sporadically dotting the sun, and their numbers change from day to day.
The ancient Chinese astronomers were among the first to observe sunspots, dating back to at least the 4th century BC. However, the first recorded telescopic observation of sunspots is attributed to Galileo Galilei in 1610.
Sunspots appear on the surface of the Sun, known as the photosphere. They are cooler, darker regions caused by intense magnetic activity, which inhibits convection and reduces surface temperature at those locations.
The sun does not have "weather" in the same way Earth does. The sun experiences phenomena like solar flares and sunspots, but these are not considered weather.