The new computer simulations are based on a magnetic field structure that is often associated with prominences: the magnetic field lines in the corona form a double arc with a small dip in the middle.
At more than one million degrees, the Sun’s atmosphere, the corona, is incredibly hot. However, not everywhere. Time and again, huge structures of significantly cooler solar plasma - about 10,000 ...
The new computer simulations are based on a magnetic field structure that is often associated with prominences: the magnetic field lines in the corona form a double arc with a small dip in the middle.
NASA’s Expedition 74 crew has progressed quantum experiments aboard the International Space Station while German researchers unveiled the most realistic simulations yet of solar prominences. The ISS ...
Scientists at the Max Planck Institute for Solar System Research have created the most realistic simulations yet of solar prominences, revealing how magnetic fields and plasma flows sustain these ...
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