Sunspots are temporary disturbances in the sun's photosphere. They appear as black spots because they are significantly cooler areas cause by magnetic activity on the sun. They can be various sizes and move across the sun at various speeds before disappearing.
Sunspots are the temporary dark spots on the surface of the sun, specifically the photosphere. Sunspots can get as big as 50,000 km long. Sunspots can interrupt terrestrial magnetism.
Sunspots are temporary disturbances on the surface of the sun that appear as darker, cooler areas caused by strong magnetic activity. They are a natural part of the solar cycle and can impact space weather by affecting solar radiation and magnetic fields.
Sunspots are temporary disturbances that appear on the surface of the Sun, specifically in its photosphere. They are cooler areas caused by magnetic activity that inhibits the flow of hot plasma, resulting in darker spots. Sunspots often occur in clusters and can vary in size and lifespan, typically appearing in an 11-year solar cycle.
Sunspots are the temporary dark spots on the surface of the sun, specifically the photosphere. Sunspots can get as big as 50,000 km long. Sunspots can interrupt terrestrial magnetism.
Dark patches on the sun's surface, known as sunspots, are areas of reduced temperature caused by magnetic activity inhibiting heat transfer. They are temporary phenomena that appear darker than their surroundings due to their cooler temperatures. Sunspots are associated with increased solar activity and can impact Earth's space weather.
Sunspots are the temporary dark spots on the surface of the sun, specifically the photosphere. Sunspots can get as big as 50,000 km long. Sunspots can interrupt terrestrial magnetism.
Sunspots are temporary disturbances on the Sun's surface that appear as dark spots due to cooler temperatures compared to the surrounding areas. They are caused by magnetic activity that inhibits convection, leading to reduced heat flow. Typically, sunspots occur in cycles that last about 11 years, correlating with the solar cycle. These phenomena can influence solar radiation and have effects on space weather and Earth's climate.
Sunspots are temporary disturbances on the surface of the sun that appear as darker, cooler areas caused by strong magnetic activity. They are a natural part of the solar cycle and can impact space weather by affecting solar radiation and magnetic fields.
Sunspots are temporary disturbances that appear on the surface of the Sun, specifically in its photosphere. They are cooler areas caused by magnetic activity that inhibits the flow of hot plasma, resulting in darker spots. Sunspots often occur in clusters and can vary in size and lifespan, typically appearing in an 11-year solar cycle.
Sunspots are the temporary dark spots on the surface of the sun, specifically the photosphere. Sunspots can get as big as 50,000 km long. Sunspots can interrupt terrestrial magnetism.
sunspots
Yes, they do.
Sunspots
Sunspots are not permanent. They are temporary. and they move once every 5 years.
it is the sunspots and thr sun is really really hot
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.
Dark patches on the sun's surface, known as sunspots, are areas of reduced temperature caused by magnetic activity inhibiting heat transfer. They are temporary phenomena that appear darker than their surroundings due to their cooler temperatures. Sunspots are associated with increased solar activity and can impact Earth's space weather.