hot bubbly plasma
The dark spots on the surface of the sun are sunspots. They are caused by intense magnetic activity which stops convection and causes a relatively cool spot.
The sun's surface and atmospheric activity are primarily driven by the interaction of magnetic fields. Magnetic fields cause regions of intense activity known as sunspots, which can lead to solar flares and coronal mass ejections. These events can impact space weather and have effects on Earth.
The phenomena occurring on the surface of the sun include sunspots, solar flares, and solar prominences. Sunspots are dark areas on the surface caused by magnetic activity, while solar flares are sudden releases of energy. Solar prominences are large loops of plasma extending from the sun's surface into its outer atmosphere.
Granulation on the Sun's surface is caused by the rising and falling of convection currents below the Sun's surface. Hot plasma rises, cools at the surface, sinks back down, and repeats this process, creating the granular pattern we observe.
Sunspotting is the activity of observing and tracking sunspots on the surface of the sun. Sunspots are dark, cooler areas on the sun's surface caused by intense magnetic activity. Tracking sunspots helps scientists study solar activity and predict space weather.
The dark spots on the surface of the sun are sunspots. They are caused by intense magnetic activity which stops convection and causes a relatively cool spot.
Dark patches on the sun's surface are known as sunspots. They appear darker because they are cooler regions on the sun's surface where magnetic activity inhibits the flow of heat. Sunspots can be large and can last for days or weeks before dissipating.
Sunspots appear cooler than the surrounding surface of the sun because they are areas of intense magnetic activity that inhibit the flow of heat from the sun's interior. This disruption in the flow of heat causes the sunspots to be cooler than their surroundings.
The Suns activity varies over time including the number of sun spots. they follow an 11 year cycle of relative activity and dormancy. At any one time there may be hundreds of them across the surface.
Sunspots are cooler areas on the sun's surface that appear darker due to intense magnetic activity. These sunspots can vary in size and can last from a few days to a few weeks before disappearing. Sunspots are typically associated with increased solar activity and can impact space weather on Earth.
Dark marks on the sun are known as sunspots. They are areas of cooler temperature on the sun's surface caused by strong magnetic activity. Sunspots can vary in size and shape and play a role in the sun's 11-year solar cycle.
Dark cool areas on the Sun's surface are called sunspots. These regions are cooler than the surrounding areas due to magnetic activity that inhibits convection, which is the process that transports heat from the Sun's interior to its surface. Sunspots can appear in groups and vary in size and duration, and they are often associated with solar activity such as solar flares and prominences.