The Maunder Minimum, a period from about 1645 to 1715 during which sunspots were notably scarce, is linked to a decrease in sunspots. This event is associated with a cooler climate period known as the "Little Ice Age."
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 most discernable features on the Sun are sunspots; areas that are a little cooler, and therefore a little darker, than the rest of the Sun around them. We know that sunspots are formed by intense magnetic regions, and that large solar flares and prominences are associated with sunspots. There's a cycle of increasing and decreasing numbers of sunspots that runs about 11 years in length, although this can vary by a couple of years. Slower cycles seem to be correlated with fewer sunspots, and faster cycles with more sunspots, but scientists don't have a detailed explanation for why the cycle exists, or why it is 11 years (more or less) in length. We are currently (in 2014) at or near the maximum of the sunspot cycle. You can see the daily view of the Sun and yesterday's sunspot number at the SpaceWeather website, www.spaceweather.com.
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 are not permanent features on the Sun. They typically last for days to weeks, and then fade away. The number of sunspots varies in an 11-year cycle known as the solar cycle.
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.
What happens when the Sun emits more energy than normal?O Solar flares and sunspots occur, increasing Earth's temperature.O Sunspots and volcanic eruptions occur, increasing Earth's temperature.O Volcanic eruptions and movement of continents occur, decreasing Earth's temperature.O Movement of continents and solar flares occurs, decreasing Earth's temperature.?
Sunspots are cooler regions on the Sun's surface, but they are associated with intense magnetic activity. While a single sunspot itself doesn't release energy like solar flares, it can be linked to larger solar phenomena that do release significant energy. Solar flares, which can occur near sunspots, can release energy equivalent to millions of hydrogen bombs, with energy outputs reaching up to 10^20 joules in a single event. Thus, while sunspots themselves aren't energy sources, their associated activities can release vast amounts of energy.
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.
In 1859, Richard Carrington observed a solar flare, which was a significant event in solar astronomy. He noted bright white light emanating from a group of sunspots, marking the first recorded observation of such an event. This solar flare was later linked to the powerful geomagnetic storm known as the Carrington Event, which caused widespread disruptions to telegraph systems on Earth. Carrington's observation provided crucial insights into solar activity and its impact on our planet.
The most discernable features on the Sun are sunspots; areas that are a little cooler, and therefore a little darker, than the rest of the Sun around them. We know that sunspots are formed by intense magnetic regions, and that large solar flares and prominences are associated with sunspots. There's a cycle of increasing and decreasing numbers of sunspots that runs about 11 years in length, although this can vary by a couple of years. Slower cycles seem to be correlated with fewer sunspots, and faster cycles with more sunspots, but scientists don't have a detailed explanation for why the cycle exists, or why it is 11 years (more or less) in length. We are currently (in 2014) at or near the maximum of the sunspot cycle. You can see the daily view of the Sun and yesterday's sunspot number at the SpaceWeather website, www.spaceweather.com.
The most discernable features on the Sun are sunspots; areas that are a little cooler, and therefore a little darker, than the rest of the Sun around them. We know that sunspots are formed by intense magnetic regions, and that large solar flares and prominences are associated with sunspots. There's a cycle of increasing and decreasing numbers of sunspots that runs about 11 years in length, although this can vary by a couple of years. Slower cycles seem to be correlated with fewer sunspots, and faster cycles with more sunspots, but scientists don't have a detailed explanation for why the cycle exists, or why it is 11 years (more or less) in length. We are currently (in 2014) at or near the maximum of the sunspot cycle. You can see the daily view of the Sun and yesterday's sunspot number at the SpaceWeather website, www.spaceweather.com.
What is true about sunspots
Sunspots are as long as your dick or vag
Galileo first discovered the sunspots in 1610.
Sunspots affect radio compunication and the 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.