LINEAR SOLAR MODELS

Solar Interface Dynamos. I. Linear, Kinematic Models in Cartesian Geometry

We describe a simple, kinematic model for a dynamo operating in the vicinity of the interface between the convective and radiative portions of the solar interior. The model dynamo resides within a Cartesian domain, partioned into an upper, convective half and lower, radiative half, with the magnetic di†usivity g of the former region assumed to exceed that of the latter The Ñuid motions that con...

Linear Models for Functional Data

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Reconstruction of Solar Coronal Linear Force-Free Magnetic Field

Standard Solar Models

A lot of progress has been made in understanding the robustness of solar model predictions since Neutrino 96 [1]. In this talk, I will first summarize the new ingredients and then give the current best-estimates. Then I will discuss the uncertainties in the predictions. Many of the results given here are adopted from the recent BP98 paper [2]. As we shall see in Section 3, there is excellent ag...

Solar Irradiance Conversion Models*