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Direct-reading Zeeman Effect Detecting Instrument
(YJS-Z)
Nine significant Zeeman splitting spectral lines can be observed
F-P clear aperture:¦Õ40mm
Fringe fineness of quartz:>12
Magnetic induction:0¡«13000GS
Central wave-length:¦Ë=546.1nm |
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Direct-reading Zeeman Effect Detecting Instrument
(YJS-ZA)
Nine significant Zeeman splitting spectral lines can be observed
F-P clear aperture:¦Õ40mm
Fringe fineness of quartz:>12
Magnetic induction:0¡«13000GS
Central wave-length:¦Ë=546.1nm
With all the CCD lens and monitors equipped
The Zeeman spllitting spectral lines can be directly observed
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Direct-reading Zeeman Effect Detecting Instrument
(YJS-ZB)
Nine significant Zeeman splitting spectral lines can be observed
F-P clear aperture:¦Õ40mm
Fringe fineness of quartz:>12
Magnetic induction:0¡«13000GS
Central wave-length:¦Ë=546.1nm
With allthe CCD lens,data acquisition card and computer equipped,the
zeeman splitting spectral lines can be directly observed and
the experimental results can be displayed through computer interface.
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Faraday Effect Detecting Instrument (WFC)
Resolution ratio of Monochromator:0.6nm
Digital displaying goniometric graduation value:1'
Digital displaying magnetic field of light:8000¡«12000GS |
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Optical Waveguide Detecting Instrument (GBG)
Beam collimating and splitting device:
Amplification ratio:1.5x
Aperture of extended parallel beam:1.2¡«1.5mm
Focal length of auxiliary lens 100mm
Goniometric rotating-disk:
Goniometric range:360¡ã
Minimum scale:6"
Goniometric precision: ¡Ü¡À15"
photoelectric detecting system:
Alignment accuracy of zero angle: ¡Ü¡À10"
Alignment accuracy of m-line synchronous angle:¡À20"
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Single-slit Diffractometer (WDY)
Minimum relative error of monochromatic wave length: ¡Ü5%
Diffraction fringe:at least ten fringes can be observed on each
side
Amplification of telescope:8x
Effective aperture of objective: ¡Ý26mm
Viewing angle:1¡ã30' |
