Abstract:
Sun’s highly inhomogeneous asymmetrical, and time dependent magnetic field plays a vital role in the non-Radiative energy transport that maintains the inhomogeneous asymmetrical and time dependent atmosphere of the sun so much hotter that the surface. Along with convection, Sun’s radiation plays an important role in maintaining the highly inhomogeneous and time dependent magnetic field of the sun. Here I briefly review our knowledge of magnetic field and rotation the two interrelated attributes of the sun on various scales.
