Zeeman-Doppler Imaging of Solar-Type Stars: Multi Line Technique

Details Zeeman-Doppler Imaging of Solar-Type Stars: Multi Line Technique Zeeman-Doppler Imaging of Solar-Type Stars: Multi Line Technique

Mar 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996soph..164..417s&link_type=abstract

Solar Physics, Volume 164, Issue 1-2, pp. 417-428

Physics

19

Solar Type Stars, Magnetic Fields, Spectropolarimetry

Scientific paper

In this work, a multi-line spectropolarimetric detection using an Echelle spectrograph 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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