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Spatial offsets between lines and continuum in limb faculae

机译:肢小结的线与连续体之间的空间偏移

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摘要

High-spatial-resolution spectra of limb faculae show spatial displacements of line cores relative to the adjacent continuum at cos θ<0.35, confirming results from earlier photographic analyses. The observed displacements are geometric measures which probe the upper atmospheric layers of fluxtubes forming facular grains. We selected spectra with highest contrast and smallest width of the facular continuum streaks, in order to avoid clustered structures. The spatial displacements of Stokes-Q and -V maxima were also measured: we find Q-signals spatially located near the continuum, as is expected from their origin in line wings; V-signals – which should give evidence for the existence of horizontal fields – are not found, except for one case of a 'hidden' pore.
机译:肢状小丘的高空间分辨率光谱显示,线芯相对于相邻连续体的空间位移在cosθ<0.35处得到证实,这证实了早期摄影分析的结果。所观察到的位移是几何量度,用于探测形成细粒的通量管的上部大气层。为了避免聚集结构,我们选择了具有最高对比度和最小的连续continu纹宽度的光谱。还测量了Stokes-Q和-V最大值的空间位移:我们发现,Q信号在空间上位于连续体附近,正如它们从线翼的起点所期望的那样;除了一个“隐藏”孔的情况外,未找到V信号-应该提供水平场存在的证据。

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  • 来源
    《Solar Physics 》 |2001年第2期| 259-268| 共10页
  • 作者

    G. Stellmacher; E. Wiehr;

  • 作者单位

    CNRS Institute d'Astrophysique;

    Universitäts-Sternwarte;

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  • 正文语种 eng
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