![Figure 1: Visualization of the temperature structure across a vertical slice through a three-dimensional (3D) model of the solar atmosphere, taken from a state-of-the-art magneto-hydrodynamic simulation of the chromosphere-corona transition region (see Ca Figure 1: Visualization of the temperature structure across a vertical slice through a three-dimensional (3D) model of the solar atmosphere, taken from a state-of-the-art magneto-hydrodynamic simulation of the chromosphere-corona transition region (see Ca](/sites/default/files/styles/crop_square_2_2_to_320px/public/images/gallery/news/prensa1489_3478.jpg?itok=qEr_1-Gs)
The CLASP suborbital rocket experiment, motivated by theoretical investigations carried out at the IAC, provided unprecedented observations of the polarization of the solar ultraviolet radiation. The theoretical modeling of these pioneering observations has revealed that the enigmatic chromosphere-corona transition region is extremely corrugated, with a geometry much more complex than in today’s most advanced models.
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