Example Data for the MARZ Magnetic Reconnection Experiments

<p>This dataset contains example data used in the MARZ magnetic reconnection expeirments.</p> <p>Experimental details are in:</p> <p>[1] R. Datta et al. (2024) PRL.&nbsp;<a href="https://doi.org/10.1103/physrevlett.132.155102" rel="nofollow">https://doi.org/10.1103/physrevlett.132.155102</a>&nbsp;<br>[2] R. Datta, et al. (2024). Phys. Plasmas.&nbsp;<a href="https://doi.org/10.1063/5.0201683" rel="nofollow">https://doi.org/10.1063/5.0201683</a></p> <p>Analysis code can be downloaded from <a href="https://github.com/ridatta/MARZ_Analysis_Tools.git">https://github.com/ridatta/MARZ_Analysis_Tools.git&nbsp;</a></p> <p>Diagnostics details are in Webb, Timothy Jay, et al. Review of Scientific Instruments 94.3 (2023).&nbsp;<a href="https://doi.org/10.1063/5.0123448" rel="nofollow">https://doi.org/10.1063/5.0123448</a></p> <p>The diagnostics in MARZ include:</p> <p>(1) B-Dots/ Inductive Probes.</p> <p>Data from each probe is stored as .CSV files.&nbsp;</p> <p>(2) Visible Spectroscopy (SVS)</p> <p>Data is stored in HDF files. For pre-processing, we need shot data, as well as calibration data, which includes pre-shot laser images, LDLS fast and slow images, and Tungsten lamp images.&nbsp;</p> <p>(3) XRS3 (X Ray Spectroscopy)</p> <p>Data is stored in TIFF files.&nbsp;</p> <p>(4) Ultra-Fast X Ray Pinhole Cameras</p> <p>Data is stored in TIFF files.&nbsp;</p> <p>(5) Self Emission Gated Optical Imager (SEGOI)</p> <p>SEGOI outputs 2D time-resolved optical emission data, and 1-D space- and time-resolved streak image data, stored in HDF5 format.</p> <p>(6) X Ray Diodes (TADPoles and LOS 170 Silicon Diodes)</p> <p>Data is stored in CSV files.&nbsp;</p>