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Stokes spectra 2014.2.23. Tetsu Anan. Before DST calibration. 20140223scan012_iquv_d.gif. After DST calibration. 20140223scan012_iquv_d_co.gif. DST calibration. Calibration by using polarization in continuum. Calibration on 2013.5.5. X N = −0.0187 、 τ N = −10.3° 、 X C = 0.0154 、
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Stokes spectra2014.2.23 Tetsu Anan
Before DST calibration 20140223scan012_iquv_d.gif
After DST calibration 20140223scan012_iquv_d_co.gif
DST calibration Calibration by using polarization in continuum Calibration on 2013.5.5 XN = −0.0187、τN = −10.3°、XC = 0.0154、 τC = −6.78°、Sc = 0 XN = −0.0200、τN = −10.3°、XC = 0.0200、 τC = −5.00°、Sc = 0 Better
After DST “re”calibration 20140223scan012_iquv_d_cn.gif
After DST “re”calibrationHigh contrast(±0.5%) 20140223scan012_iquv_d_cn_2.gif
Continuum offsetHigh contrast(±0.5%) 20140223scan012_iquv_d_cn_con.gif refer to polarization in continuum between white lines
Remove fringe, Casini’s methodHigh contrast(±0.5%) 20140223scan012_iquv_d_cn_con_casini1.gif
Remove fringe, Casini’s methodHigh contrast(±0.1%) 20140223scan012_iquv_d_cn_con_casini1_1.gif
Remove fringe, Casini’smethod、SiHigh contrast(±0.5%) 20140223scan012_iquv_d_cn_con_casini1si.gif
Summary • Save data • He : 20140526_7.sav • Si : 20140527_1.sav
Sign of V • NOAA11982、黒点は波長短い方が負