According to the measuring results with the Kitt Peak Fourier spectrometer, a net circular polarization causing Stocks Ⅴ asymmetry in each spectral lines was discovered in a broad-band spectrum region, i.e. the white...According to the measuring results with the Kitt Peak Fourier spectrometer, a net circular polarization causing Stocks Ⅴ asymmetry in each spectral lines was discovered in a broad-band spectrum region, i.e. the white light. The bluewing polarization peak is always larger in amplitude and area than the red-wing one.展开更多
On duly 23, 1987, at about 06h UT by means of Solar Magnetic Field Telescope with a new CCD camera and image processor, which can be used for the measure- ments of the solar vector magnetic field and the sight line ve...On duly 23, 1987, at about 06h UT by means of Solar Magnetic Field Telescope with a new CCD camera and image processor, which can be used for the measure- ments of the solar vector magnetic field and the sight line velocity field in both photosphere (λ5324(?)) and the chromosphere (λ4861(?)), a series of data of the magnetic fields and the sight line velocity fields are obtained in No. 87036展开更多
文摘According to the measuring results with the Kitt Peak Fourier spectrometer, a net circular polarization causing Stocks Ⅴ asymmetry in each spectral lines was discovered in a broad-band spectrum region, i.e. the white light. The bluewing polarization peak is always larger in amplitude and area than the red-wing one.
文摘On duly 23, 1987, at about 06h UT by means of Solar Magnetic Field Telescope with a new CCD camera and image processor, which can be used for the measure- ments of the solar vector magnetic field and the sight line velocity field in both photosphere (λ5324(?)) and the chromosphere (λ4861(?)), a series of data of the magnetic fields and the sight line velocity fields are obtained in No. 87036
