Seifert Maria, Weule Mareike, Cipiccia Silvia, Flenner Silja, Hagemann Johannes, Ludwig Veronika, Michel Thilo, Neumayer Paul, Schuster Max, Wolf Andreas, Anton Gisela, Funk Stefan, Akstaller Bernhard
ECAP, Friedrich-Alexander-Universität Erlangen-Nürnberg, Erwin-Rommel-Str. 1, 91058 Erlangen, Germany.
Diamond Light Source Ltd., Diamond House, Harwell Science and Innovation Campus, Didcot, Oxfordshire OX11 0DE, UK.
J Imaging. 2020 Jul 3;6(7):63. doi: 10.3390/jimaging6070063.
For imaging events of extremely short duration, like shock waves or explosions, it is necessary to be able to image the object with a single-shot exposure. A suitable setup is given by a laser-induced X-ray source such as the one that can be found at GSI (Helmholtzzentrum für Schwerionenforschung GmbH) in Darmstadt (Society for Heavy Ion Research), Germany. There, it is possible to direct a pulse from the high-energy laser Petawatt High Energy Laser for Heavy Ion eXperiments (PHELIX) on a tungsten wire to generate a picosecond polychromatic X-ray pulse, called backlighter. For grating-based single-shot phase-contrast imaging of shock waves or exploding wires, it is important to know the weighted mean energy of the X-ray spectrum for choosing a suitable setup. In propagation-based phase-contrast imaging the knowledge of the weighted mean energy is necessary to be able to reconstruct quantitative phase images of unknown objects. Hence, we developed a method to evaluate the weighted mean energy of the X-ray backlighter spectrum using propagation-based phase-contrast images. In a first step wave-field simulations are performed to verify the results. Furthermore, our evaluation is cross-checked with monochromatic synchrotron measurements with known energy at Diamond Light Source (DLS, Didcot, UK) for proof of concepts.
对于持续时间极短的成像事件,如冲击波或爆炸,必须能够通过单次曝光对物体进行成像。一种合适的装置是由激光诱导X射线源提供的,例如在德国达姆施塔特的GSI(亥姆霍兹重离子研究中心有限公司,重离子研究协会)可以找到的那种。在那里,可以将来自用于重离子实验的高能激光拍瓦级高能激光(PHELIX)的脉冲导向钨丝,以产生皮秒级多色X射线脉冲,称为背光源。对于基于光栅的冲击波或爆炸丝的单次相衬成像,了解X射线光谱的加权平均能量对于选择合适的装置很重要。在基于传播的相衬成像中,了解加权平均能量对于能够重建未知物体的定量相图像是必要的。因此,我们开发了一种使用基于传播的相衬图像来评估X射线背光源光谱加权平均能量的方法。第一步是进行波场模拟以验证结果。此外,我们的评估通过在英国迪德科特的钻石光源(DLS)进行的已知能量的单色同步加速器测量进行交叉核对,以验证概念。