A dynamo scenario for polar and whole-surface starspot generation

Rapidly rotating young (T Tauri, pre-Main-Sequence, and Main-Sequence) star s as well as subgiants seem to show starspots not only at low and middle la titudes, as the Sun, but also at high latitudes and even around the poles. We consider a simple nonlinear Parker migratory dynamo model working in a t hin shell in order to investigate how high latitude and polar spots may be produced for different values of the dynamo layer radius and thickness and for various rotation rates. Simple assumptions on the angular velocity grad ient and helicity distribution are made according to symmetry properties an d recent solar and stellar observations. A recently proposed asymptotic WKB -type approach is used to solve the dynamo problem and its drawbacks and ad vantages in the solar and stellar contexts are discussed. As a general resu lt, we find that a sizable toroidal field can be produced over a much more extended latitude range than in the Sun, thus explaining in a natural way t he occurrence of activity from the poles to the equator in such stars. Our approach complements that proposed by Schussler et al. (1996) which is focu sed on the instability and emergence of the azimuthal flux tubes, as well a s the analyses based on a dynamo working over an extended part of the stell ar convective envelope (Moss, Tuominen, and Brandenburg, 1991; Moss et al., 1995).