Prominence
The loops of gas found on the sun are called solar prominences. They are large, bright features that extend out from the sun's surface into its outer atmosphere, known as the corona, and are typically associated with the sun's magnetic field.
The phenomenon described is a solar flare. Solar flares are intense bursts of energy emitted from the sun's surface, which can produce dramatic loops or arches of gas suspended in the sun's atmosphere.
solar storms the large bright loops are called solar flares solar prominence A+
Solar prominences are huge bursts of gas that erupt from the sun's atmosphere and form enormous loops due to the sun's magnetic field. These loops can extend tens of thousands of kilometers into space and can last for several hours to even months before dissipating. Solar prominences are often associated with solar flares and can release large amounts of energy and particles into space.
The fiery arms or loops extending from the sun's surface are called solar prominences. These are large, bright features that extend outward from the sun's surface, often in a loop shape, and are composed of plasma. Solar prominences are associated with the sun's magnetic field and can last for several hours to days before dissipating.
Prominence
The streams of charged particles flowing out into Space from the Sun are collectively the Solar Wind.
Prominances these are loops , Solar Flares these are matter ejections from the sun, and sunspots these are the darker cooler places on its surface
loops of fire that burst from the sun of course
Loops of PlasmaAnchored in the photosphere, these coronal loops measure up to 60,000 miles and can be observed between the lower corona and the transition region of the Sun. Flowing along the magnetic field, the arches begin to rise when the plasma heats up, and crash down when it cools at more than 60 miles per second. Scientists have recently suggested that they heat the corona to temperatures about 300 times the sun's surface.
More coils of wire around the magnetic material.More current through the wire in the coil.Increasing the current flowing through the wire Increasing the number of loops of wireputting a piece of iron inside the loops of wire apex :)Increasing the current flowing through the wireIncreasing the number of loops of wire
Prominences
Prominences
The loops of gas found on the sun are called solar prominences. They are large, bright features that extend out from the sun's surface into its outer atmosphere, known as the corona, and are typically associated with the sun's magnetic field.
The layer of the Sun where eruptions occur due to the sudden connection of loops in sunspot regions is the corona. These eruptions, known as solar flares, are caused by the release of magnetic energy stored in the corona. The interactions and reconnections of magnetic field lines in this outer atmosphere can lead to significant bursts of energy and matter into space.
Solar flares are blasts of gas from the sun's atmosphere that can form enormous loops due to the sun's magnetic field. These loops are known as coronal loops and can span many times the diameter of the Earth. Solar flares can release massive amounts of energy and particles into space.
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