Theory of line formation depth and its application. (I): The contribution function and the line formation depth.

Astronomy and Astrophysics – Astronomy

Scientific paper

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Line Formation: Radiative Transfer, Solar Magnetic Fields: Structure

Scientific paper

The development and new progress of the theory of line formation depth with its related contribution and response functions are stated in this series of papers, while the recent work is emphasized. The application of the theory, especially, to the derivation of the structure of solar vector magnetic fields is presented. In this first paper, the theory concerning the contribution function, its limitation and the issue of uniqueness are discussed.

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