Introduction

Abstract

AbstractUnderstanding the self-consistent coupling and flow of energy, momentum, matter, and electromagnetic fields is necessary for every aspect of solar, space, and astrophysics. Transport of energy from the center of Sun or a star to the photosphere determines its stellar evolution, for example. The transport of convective energy and its translation to magnetic energy and the subsequent transport of magnetic energy into the solar corona is thought to be responsible for the unexpected heating of the solar corona to its very high temperatures. The transport of mass, momentum, and energy is necessary to understand the physics of expanding flows, such as the solar wind and stellar winds, the interstellar medium, and almost every conceivable flow found in a solar, space, and astrophysics context.KeywordsSolar WindTransport CoefficientOuter HeliosphereLocal Interstellar MediumDiffusive Shock AccelerationThese keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.