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Fiber-Optic Magnetometer for Prime Focus of 6-m BTA Telescope Basedon Suspended Echelle Spectrograph

机译:基于悬浮埃歇尔光谱仪的6米BTA望远镜主要焦点的光纤磁力计

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We have developed and manufactured a fiber-optic magnetometer for the prime focus of the6-m BTA telescope of the Special Astrophysical Observatory of the Russian Academy of Sciences basedon a suspended echelle spectrograph. The magnetometer is designed to improve the spectrum stabilityand eliminate the effect of instrumental polarization of the diagonal mirror on the results of magnetic fieldmeasurements. The magnetometer is to be used for measurements of stellar magnetic fields in stars and to study their chemical composition. The instrument operates in the 5000-6800 A wavelength interval withmean reciprocal dispersion of 0.15 A/pixel. According to the estimates for 9m.5 stars, the standard error ofmagnetic field measurements based on 400 spectral lines would be 100 G for a half-hour exposure.
机译:我们已经开发并制造了一种光纤磁强计,用于基于悬浮式埃歇尔光谱仪的俄罗斯科学院特殊天文台的6米BTA望远镜的主要焦点。磁力计旨在提高频谱稳定性,并消除对角镜的仪器极化对磁场测量结果的影响。磁力计将用于测量恒星中的恒星磁场并研究其化学成分。该仪器在5000-6800 A的波长范围内工作,平均色散为0.15 A /像素。根据对9m.5星的估计,半小时曝光基于400条谱线的磁场测量的标准误差为100G。

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