Nave Colin
Diamond Light Source Ltd, Harwell Science and Innovation Campus, Didcot OX11 0DE, UK.
J Synchrotron Radiat. 2018 Sep 1;25(Pt 5):1490-1504. doi: 10.1107/S1600577518009566. Epub 2018 Aug 27.
X-ray imaging allows biological cells to be examined at a higher resolution than possible with visible light and without some of the preparation difficulties associated with electron microscopy of thick samples. The most used and developed technique is absorption contrast imaging in the water window which exploits the contrast between carbon and oxygen at an energy of around 500 eV. A variety of phase contrast techniques are also being developed. In general these operate at a higher energy, enabling thicker cells to be examined and, in some cases, can be combined with X-ray fluorescence imaging to locate specific metals. The various methods are based on the differences between the complex refractive indices of the cellular components and the surrounding cytosol or nucleosol, the fluids present in the cellular cytoplasm and nucleus. The refractive indices can be calculated from the atomic composition and density of the components. These in turn can be obtained from published measurements using techniques such as chemical analysis, scanning electron microscopy and X-ray imaging at selected energies. As examples, the refractive indices of heterochromatin, inner mitochondrial membranes, the neutral core of lipid droplets, starch granules, cytosol and nucleosol are calculated. The refractive index calculations enable the required doses and fluences to be obtained to provide images with sufficient statistical significance, for X-ray energies between 200 and 4000 eV. The statistical significance (e.g. the Rose criterion) for various requirements is discussed. The calculations reveal why some cellular components are more visible by absorption contrast and why much greater exposure times are required to see some cellular components. A comparison of phase contrast as a function of photon energy with absorption contrast in the water window is provided and it is shown that much higher doses are generally required for the phase contrast measurements. This particularly applies to those components with a high carbon content but with a mass density similar to the surrounding cytosol or nucleosol. The results provide guidance for the most appropriate conditions for X-ray imaging of individual cellular components within cells of various thicknesses.
X射线成像能够以比可见光更高的分辨率对生物细胞进行检测,而且不存在与厚样品电子显微镜相关的一些制备难题。最常用且发展最成熟的技术是水窗吸收对比成像,它利用了碳和氧在约500电子伏特能量下的对比度。各种相衬技术也在不断发展。一般来说,这些技术在更高的能量下运行,能够检测更厚的细胞,并且在某些情况下,可以与X射线荧光成像相结合来定位特定金属。各种方法基于细胞成分与周围细胞质或核质(存在于细胞细胞质和细胞核中的流体)的复折射率差异。复折射率可以根据成分的原子组成和密度来计算。这些又可以通过使用化学分析、扫描电子显微镜和选定能量下的X射线成像等技术的已发表测量结果来获得。例如,计算了异染色质、线粒体内膜、脂滴的中性核心、淀粉颗粒、细胞质和核质的折射率。折射率计算能够获得所需的剂量和注量,以在200至4000电子伏特的X射线能量下提供具有足够统计显著性的图像。讨论了各种要求下的统计显著性(例如罗斯准则)。计算结果揭示了为什么一些细胞成分通过吸收对比更明显,以及为什么观察某些细胞成分需要更长的曝光时间。提供了作为光子能量函数的相衬与水窗吸收对比的比较,结果表明相衬测量通常需要高得多的剂量。这尤其适用于那些碳含量高但质量密度与周围细胞质或核质相似的成分。研究结果为在不同厚度细胞内对单个细胞成分进行X射线成像的最合适条件提供了指导。