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Table of Contents
Preface
Reconstructing images in astrophysics, an inverse problem point of view
Reconstruction of the solar subsurface through helioseismology with SDO
Imaging surface spots from space-borne photometry
Reconstruction of Thermal and Magnetic Field Structure of the Solar Subsurface through Helioseismology
Physical processes leading to surface inhomogeneities: the case of rotation
Interferometry to determine stellar shapes: application to Achernar
Interferometry to image surface spots
Interferometric Surface Mapping of RapidlyRotating Stars.
Application to the Be star Achernar
Doppler and Zeeman Doppler Imaging of Stars.
Reconstructing images in astrophysics, an inverse problem point of view
Reconstruction of the solar subsurface through helioseismology with SDO
Imaging surface spots from space-borne photometry
Reconstruction of Thermal and Magnetic Field Structure of the Solar Subsurface through Helioseismology
Physical processes leading to surface inhomogeneities: the case of rotation
Interferometry to determine stellar shapes: application to Achernar
Interferometry to image surface spots
Interferometric Surface Mapping of RapidlyRotating Stars.
Application to the Be star Achernar
Doppler and Zeeman Doppler Imaging of Stars.