Data from: An implicit, conservative electrostatic particle-in-cell algorithm for paraxial magnetic nozzles
Authors/Creators
- 1. Universidad Carlos III de Madrid
- 2. Los Alamos National Laboratory
Description
# Data from: Plasma acceleration in a magnetic arch
- Authors: Mario Merino, Diego García, Eduardo Ahedo
- Contact email: pejimene@ing.uc3m.es
- Date: 2023-06-26
- Keywords: electric propulsion, plasma simulation, magnetic nozzles, implicit particle-in-cell (PIC)
- Version: 0.1
- Digital Object Identifier (DOI): 10.5281/zenodo.8081963
- License: This dataset is made available under the [Open Data Commons Attribution License](http://opendatacommons.org/licenses/by/1.0/)
## Abstract
This dataset contains the data found in the plots of the preprint:
_[Pedro Jimenez, Luis Chacon, Mario Merino, "An implicit, conservative electrostatic particle-in-cell algorithm for paraxial magnetic nozzles", arxiv.org](https://arxiv.org/pdf/2305.07146.pdf)._
The data in this repository has been extracted from kinetic simulations as described in the reference. For further information on the setup for the simulation please refer to the article.
## Data files
The data files are in .csv format. They were produced in Julia using _[CSV.jl](https://csv.juliadata.org/stable/)_ and _[DataFrames.jl](https://dataframes.juliadata.org/stable/) libraries.
The files are organised following the order of the figures in the article. All the plots are 1D series, the first column corresponding to the x-axis data. Y-axis data is presented in the following columns, the total number of columns equal to the number of line series in the plot +1. The title of each series is found in the first row of the .csv files. Please find below some specificalities in certain figures:
- The columns for the time evolution in **fig6_left.csv** and **fig6_right.csv** (corresponding to the actual left and right columns in the figure i.e. cases A and B) contain a field tag followed by the corresponding time step (e.g. phi_500).
- Due to the different number of nodes, steady state fields for cases A and B are saved in **fig8_a-f.csv** while cases AF and BF are saved in **fig8_a-f_fine.csv**.
The rest of the data files should be self descripting
## Citation
Any works using this dataset or any part of it in any form shall cite it as follows:
The prefered means of citation is to reference the publication asociated to the dataset with DOI: 10.1088/1361-6595/acd476
The BibTex is also provided for the sake of convinience:
@article{Merino_2023,
doi = {10.1088/1361-6595/acd476},
url = {https://dx.doi.org/10.1088/1361-6595/acd476},
year = {2023},
month = {jun},
publisher = {IOP Publishing},
volume = {32},
number = {6},
pages = {065005},
author = {Mario Merino and Diego García-Lahuerta and Eduardo Ahedo},
title = {Plasma acceleration in a magnetic arch},
journal = {Plasma Sources Science and Technology},
abstract = {}
}
Optionally the dataset can be cited by referencing the DOI: 10.5281/zenodo.7947735
[](https://doi.org/10.5281/zenodo.7947735)
## Acknowledgments
This dataset was created by the [ERC-ZARATHUSTRA project](https://erc-zarathustra.uc3m.es/).
The ERC-ZARATHUSTRA project has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (grant agreement No 950466).
Files
fig10_a.csv
Files
(288.5 kB)
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Additional details
Related works
- Is described by
- Journal article: 10.48550/arXiv.2305.07146 (DOI)
Funding
References
- Jimenez et al. (2023). [arXiv:2305.07146]