Table of Contents
Spot mapping in cool stars
Science goals
Doppler Imaging I: Basic Principles
PPT Slide
PPT Slide
PPT Slide
Data requirements
Combining line profiles
LSD profiles of Gl 176.3 and AB Dor
Time series: deconvolved Stokes I profiles
Choice of mapping parameter
Local specific intensities
Image-data transformation
Regularised least-squares solutions
Regularised least-squares strategies
RX J1508.6 -4423
Dealing with nuisance parameters
A more systematic approach
Heterogeneous datasets
Surface resolution and noise
Surface resolution and noise – 2
The Occamian approach
Future prospects: The perfect spot code
Starspots as flow tracers
Surface shear: 1996 December 23 - 29
Data-space fits to differential rotation
Spot lifetimes: dwarfs vs (sub)giants
Do spots drift poleward on HR 1099?
So how far have we got?
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Author: Physics & Astronomy
Email: acc4@st-and.ac.uk
Home Page: http://star-www.st-and.ac.uk/~acc4/homepage.html
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