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Connection Between Chromospheric Events and Photospheric Dynamics

机译:大气层事件与光层动力学之间的联系

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摘要

We analyzed chromospheric events and their connection to oscillation phenomena and photospheric dynamics. The observations were done with the New Solar Telescope of Big Bear Solar Observatory using a broad-band imager at the wavelength of a TiO band and FISS spectrograph scanning Ca ii and Hα spectral lines. The event in Ca ii showed strong plasma flows and propagating waves in the chromosphere. The movement of the footpoints of flux tubes in the photosphere indicated flux tube entanglement and magnetic reconnection as a possible cause of the observed brightening and waves propagating in the chromosphere. An upward propagating train of waves was observed at the site of the downflow event in Hα. There was no clear relationship between photospheric waves and the Ca ii and Hα events. Our observations indicate that chromospheric waves that were previously thought to originate from the photosphere may be generated by some events in the chromosphere as well.
机译:我们分析了色球层事件及其与振荡现象和光球动力学的联系。观测是用大熊太阳天文台的新太阳望远镜使用的宽带成像仪在TiO波段波长下进行的,并用FISS光谱仪扫描了Ca ii和Hα谱线。 Ca ii事件表明色球层中强烈的等离子体流动和传播波。光通量管中光通量管脚点的移动表明,光通量管缠结和磁重联是观察到的变色和波在色球中传播的可能原因。在Hα的降流事件现场观察到了向上传播的波列。光球波与Ca ii和Hα事件之间没有明确的关系。我们的观察结果表明,以前认为是由光球产生的色球波也可能是由色球层中的某些事件产生的。

著录项

  • 来源
    《Solar Physics 》 |2013年第1期| 55-71| 共17页
  • 作者单位

    Department of Astronomy New Mexico State University">(1);

    Big Bear Solar Observatory">(2);

    Astronomy Program Department of Physics and Astronomy Seoul National University">(3);

    Astronomy Program Department of Physics and Astronomy Seoul National University">(3);

    Astronomy Program Department of Physics and Astronomy Seoul National University">(3);

    Big Bear Solar Observatory">(2);

    Big Bear Solar Observatory">(2);

    Astronomy Program Department of Physics and Astronomy Seoul National University">(3);

  • 收录信息
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

    Chromosphere; Photosphere;

    机译:色球光球;

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