Solar Surface Convection | Living Reviews in Solar Physics Skip to main content SpringerLink
Account Menu Find a journal Publish with us Track your research Search Cart 1.Home 2.Living …

The quiet Sun is the region of the solar surface outside of sunspots, pores, and plages. In
continuum intensity it appears dominated by granular convection. However, in polarized …

I have felt the need for a book on the theory of solar magnetic fields for some time now. Most
books about the Sun are written by observers or by theorists from other branches of solar …

A wealth of new experimental and theoretical results has been obtained in solar physics
since the first edition of this textbook appeared in 1989. Thus all nine chapters have been …

A powerful cross-correlation method for the precise measurement of the proper motion of
tracers seen on successive images of a time series of solar granulation is proposed. The …

The past few decades have seen dramatic progress in our understanding of solar interior
dynamics, prompted by the relatively new science of helioseismology and increasingly …

The Sun's axisymmetric large-scale flows, differential rotation and meridional circulation, are
thought to be maintained by the influence of rotation on the thermal-convective motions in …

Topology of convection beneath the solar surface ADS Classic is now deprecated. It will be
completely retired in October 2019. This page will automatically redirect to the new ADS interface …

The Sun's supergranulation refers to a physical pattern covering the surface of the quiet Sun
with a typical horizontal scale of approximately 30,000 km and a lifetime of around 1.8 d. Its …

In this chapter we will briefly review the basic interactions between particles and magnetic
fields, the processes that occur on the Sun which are relevant for space weather as well as …