Abstract
In this work, a multi-line spectropolarimetric detection using an Echelle spec-trograph is described. The polarization of Zeeman effect is detected by the use of more than 200 lines observed in the solar type star, HR1099. Using the statistics analysis in a sample of 200 lines, we found on the average a polarization signal of about 3 × 10−4.
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References
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© 1996 Kluwer Academic Publishers
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Semel, M., Li, J. (1996). Zeeman-Doppler Imaging of Solar-Type Stars: Multi Line Technique. In: Stenflo, J.O., Nagendra, K.N. (eds) Solar Polarization. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-0231-2_35
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DOI: https://doi.org/10.1007/978-94-009-0231-2_35
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-6586-3
Online ISBN: 978-94-009-0231-2
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