Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997pabei..15...98q&link_type=abstract
Prog. Astron., Vol. 15, No. 2, p. 98 - 111
Astronomy and Astrophysics
Astronomy
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.
Chen Xuekun
Ding Youji
Qu Zhongquan
Zhang Xiaoyu
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