Solar Photosphere: Structure, Convection, and Magnetic Fi...
Stenflo, Jan Olof![Solar Photosphere: Structure, Convection, and Magnetic Fields](https://support.digitalhusky.com/media/annotations/sorted/154/15457844/CHSBZCOP0315457844.jpg)
Solar and stellar photospheres constitute the layers most accessible to observations, forming the interface between the interior and the outside of the stars. The solar atmosphere is a rich physics laboratory, in which the whole spectrum of radiative, dynamical, and magnetic processes that tranfer energy into space can be observed. As the fundamental processes take place on very small spatial scales, we need high· resolution observations to ex...