They run the simulation and change several parameters to see how the choice of parameters affects the simulation. They look for the right shape of the structures described above. For the right shapes, the jet is an efficient engine. A scientist can explore and walk inside 1CRN-crambin, a small protein consisting of 327 atoms. These can be seen from the earth against the limb of the sun.
Prominences are important because they affect communications and surveillance satellites.
The force lifting this huge mass of plasma so high against the force of gravity is the solar magnetic field. This visualization shows the essential physics for the support process of a solar prominence. The overlying curved lines are the polar magnetic field lines. The underlying lines are the ones that produce and can support the mass of the prominences against solar gravitation. The image shows the 3D reconstruction of a microstructure from a high-purity steel sample.