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thesis.out
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\BOOKMARK [0][]{chapter*.2}{Summary}{}
\BOOKMARK [0][]{chapter.1}{1 Introduction}{}
\BOOKMARK [1][]{section.1.1}{1.1 The Sun}{chapter.1}
\BOOKMARK [1][]{section.1.2}{1.2 The chromosphere}{chapter.1}
\BOOKMARK [1][]{section.1.3}{1.3 Aim and outline of this work}{chapter.1}
\BOOKMARK [0][]{chapter.2}{2 Spectral lines}{}
\BOOKMARK [1][]{section.2.1}{2.1 Radiative transfer and spectral line formation}{chapter.2}
\BOOKMARK [1][]{section.2.2}{2.2 Hydrogen Balmer- line \(H\)}{chapter.2}
\BOOKMARK [1][]{section.2.3}{2.3 Hei 10830 \305 multiplet }{chapter.2}
\BOOKMARK [0][]{chapter.3}{3 Observations}{}
\BOOKMARK [1][]{section.3.1}{3.1 Angular resolution and Seeing}{chapter.3}
\BOOKMARK [1][]{section.3.2}{3.2 Telescope}{chapter.3}
\BOOKMARK [2][]{subsection.3.2.1}{3.2.1 Kiepenheuer Adaptive Optics System}{section.3.2}
\BOOKMARK [1][]{section.3.3}{3.3 High spatial resolution}{chapter.3}
\BOOKMARK [2][]{subsection.3.3.1}{3.3.1 Instrument}{section.3.3}
\BOOKMARK [2][]{subsection.3.3.2}{3.3.2 Observations}{section.3.3}
\BOOKMARK [2][]{subsection.3.3.3}{3.3.3 Data reduction}{section.3.3}
\BOOKMARK [3][]{subsubsection.3.3.3.1}{3.3.3.a Speckle interferometry of the broadband images}{subsection.3.3.3}
\BOOKMARK [3][]{subsubsection.3.3.3.2}{3.3.3.b Speckle reconstruction of the narrow-band images}{subsection.3.3.3}
\BOOKMARK [3][]{subsubsection.3.3.3.3}{3.3.3.c Multi object multi frame blind deconvolution}{subsection.3.3.3}
\BOOKMARK [1][]{section.3.4}{3.4 Infrared spectrometry}{chapter.3}
\BOOKMARK [2][]{subsection.3.4.1}{3.4.1 Instrument}{section.3.4}
\BOOKMARK [2][]{subsection.3.4.2}{3.4.2 Observations}{section.3.4}
\BOOKMARK [2][]{subsection.3.4.3}{3.4.3 Data reduction}{section.3.4}
\BOOKMARK [0][]{chapter.4}{4 High resolution imaging of the chromosphere}{}
\BOOKMARK [1][]{section.4.1}{4.1 Dark clouds}{chapter.4}
\BOOKMARK [1][]{section.4.2}{4.2 Fast events and waves}{chapter.4}
\BOOKMARK [2][]{subsection.4.2.1}{4.2.1 Observations and data reduction}{section.4.2}
\BOOKMARK [2][]{subsection.4.2.2}{4.2.2 Physical parameters}{section.4.2}
\BOOKMARK [2][]{subsection.4.2.3}{4.2.3 Fast events in H}{section.4.2}
\BOOKMARK [2][]{subsection.4.2.4}{4.2.4 Magnetoacoustic waves}{section.4.2}
\BOOKMARK [2][]{subsection.4.2.5}{4.2.5 Summary on some properties of the active chromosphere}{section.4.2}
\BOOKMARK [1][]{section.4.3}{4.3 Comparison between speckle interferometry and blind deconvolution }{chapter.4}
\BOOKMARK [0][]{chapter.5}{5 Spicules at the limb}{}
\BOOKMARK [1][]{section.5.1}{5.1 Spicule emission profiles observed in Hei 10830 \305}{chapter.5}
\BOOKMARK [2][]{subsection.5.1.1}{5.1.1 Observational intensity profiles and intensity ratio}{section.5.1}
\BOOKMARK [2][]{subsection.5.1.2}{5.1.2 Results}{section.5.1}
\BOOKMARK [2][]{subsection.5.1.3}{5.1.3 Conclusions}{section.5.1}
\BOOKMARK [1][]{section.5.2}{5.2 High resolution imaging of spicules}{chapter.5}
\BOOKMARK [0][]{chapter.6}{6 Conclusions and outlook }{}
\BOOKMARK [0][]{section*.27}{Bibliography}{}
\BOOKMARK [0][]{chapter*.28}{Publications}{}
\BOOKMARK [0][]{chapter*.29}{Acknowledgements}{}
\BOOKMARK [0][]{chapter*.30}{Lebenslauf}{}