Sunspots occur on the Sun due to magnetic activity that inhibits the convection process in the Sun's outer layer, the photosphere. These areas are cooler than their surroundings, leading to a darker appearance. The magnetic fields associated with sunspots can become very strong, which is linked to the solar cycle, causing fluctuations in their number and size over approximately an 11-year period.
What is true about sunspots
They appear in the Photosphere. That's basically the "surface" of the Sun.
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.
I believe that the layer in which sun spots occur would be the chromosphere. The chromosphere is the second layer in the sun's atmosphere and is about 2,000km above the photosphere(the first layer).
Sunspots are caused by interactions between the Sun's magnetic field and its plasma. Magnetic field lines become twisted and concentrated, inhibiting the flow of energy from within the Sun, resulting in cooler and darker regions on the surface known as sunspots. These sunspots appear darker because they are cooler compared to the surrounding areas.
What is true about sunspots
I assume you are talking about sunspots, as they are, in effect, "storms on the sun". They occur on or near the sun's surface.
They appear in the Photosphere. That's basically the "surface" of the Sun.
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.
I believe that the layer in which sun spots occur would be the chromosphere. The chromosphere is the second layer in the sun's atmosphere and is about 2,000km above the photosphere(the first layer).
A sunspot is a region on the Sun's photosphere that is cooler and darker than the surrounding material. Sunspots often appear in pairs or groups with specific magnetic polarities that indicate electromagnetic origins.
Sunspots are caused by interactions between the Sun's magnetic field and its plasma. Magnetic field lines become twisted and concentrated, inhibiting the flow of energy from within the Sun, resulting in cooler and darker regions on the surface known as sunspots. These sunspots appear darker because they are cooler compared to the surrounding areas.
Sun spots and prominences.
Dark areas on the photosphere of the Sun are called sunspots. They appear dark because they are cooler regions compared to their surrounding areas, which results in decreased luminosity. Sunspots are temporary phenomena that occur in 11-year cycles as part of the Sun's magnetic activity.
Sunspots are cooler regions of the Sun's surface (they are still really bright, they just look dark compared to the surrounding Sun) they are caused by what are basically magnetic field "tangles" stopping the convection that brings heat to the solar surface.
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.
Solar flares occur near regions of sunspots because sunspots are areas of intense magnetic activity on the Sun's surface. These strong magnetic fields can become twisted and tangled, leading to the release of energy in the form of solar flares. The interaction between magnetic fields in sunspots creates conditions that are conducive to the occurrence of solar flares.