Well,you don't really know.
Streams of protons and electrons emitted from the Sun produce solar wind, a continuous flow of charged particles that sweep through the solar system. These particles can interact with the magnetic field of Earth, causing phenomena such as auroras and geomagnetic storms.
The four main types of sun storms are solar flares, coronal mass ejections (CMEs), solar wind, and solar energetic particle events. These sun storms can have various impacts on Earth's space weather and technology.
Solar flares: intense bursts of radiation emitted from the sun's surface. Coronal mass ejections (CMEs): massive expulsions of plasma and magnetic field from the sun's corona. Solar particle events: high-energy particles released from the sun that can impact satellites and astronauts in space.
solar storms or winds hit the ozone
Solar flares from the sun produce bursts of solar wind, but solar wind is constantly streaming out from the sun.
They are called solar prominences.
The solar wind originates from the outermost layer of the Sun called the corona, which is the Sun's tenuous outer atmosphere. The corona is made up of highly ionized gas that is so hot it can escape the Sun's gravitational pull and flow outwards into space, creating the solar wind.
Storms on the surface of the sun, known as solar storms, primarily include solar flares and coronal mass ejections (CMEs). Solar flares are intense bursts of radiation caused by the release of magnetic energy, while CMEs involve the ejection of large quantities of plasma and magnetic field from the sun's corona. These storms can impact space weather, affecting satellite operations, communication systems, and even power grids on Earth. They are driven by the sun's magnetic activity and cycles, particularly during solar maximum periods.
Capture the sun
Geomagnetic storms are disturbances in the Earth's magnetosphere caused by solar wind interacting with the Earth's magnetic field. These storms can result in enhanced auroras, disruptions to satellite and radio communications, and potential damage to power grids. They are often brought on by solar flares or coronal mass ejections from the sun.
Solar storms can affect the space environment around the moon, leading to increased radiation levels and potential disruption of communication signals. The moon has no magnetic field to shield it from solar winds and energetic particles, making it more vulnerable to the effects of solar storms.
sunspots prominence solar flares solar winds