![In the image above obtained with the NASA’s spectrograph IRIS, can be seen in the bedge or limbo of the Sun the multitude of jets leaping the surface. In the center image, the numerical model is able to reproduce the jets. In the image below, taken with
In the image above obtained with the NASA’s spectrograph IRIS, can be seen in the bedge or limbo of the Sun the multitude of jets leaping the surface. In the center image, the numerical model is able to reproduce the jets. In the image below, taken with](/sites/default/files/styles/crop_square_2_2_to_320px/public/images/gallery/news/prensa1220_2639.jpg?itok=6oEPBxLt)
Combining computer observations and simulations, a new model shows that the presence of neutrals in the gas facilitates the magnetic fields to penetrate through the surface of the Sun producing the spicules. In this study, led by an astrophysicist who studied at the University of La Laguna, participated the Swedish Solar Telescope of the Roque de los Muchachos Observatory in La Palma.
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