Sunspots are temporary phenomena on the surface of the Sun. The number vary over time, but there is a "trend" towards a greater number appearing every eleven years. However, this "trend" seems to be "disturbed" as the "11 year" cycle is very late.
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You can see today's (well, yesterday's) sunspot numbers each day at www.spaceweather.com, or click the link below.
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
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.
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).
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 appear on the surface of the Sun, specifically in the photosphere. These darker, cooler areas are caused by magnetic activity on the Sun's surface. Sunspots can vary in size and shape and are often seen in groups.
Sunspots are areas on the sun's surface that appear darker than their surroundings due to cooler temperatures. They are caused by strong magnetic activity and can vary in size, shape, and intensity. Sunspots are often accompanied by solar flares and coronal mass ejections.
Sunspots are structures commonly found in the photosphere of the Sun. These dark regions are caused by magnetic activity and are cooler than the surrounding areas, hence appearing dark against the brighter photosphere. Sunspots often occur in pairs with opposite magnetic polarities.