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Published June 26, 2023 | Version 0.1

Data from: An implicit, conservative electrostatic particle-in-cell algorithm for paraxial magnetic nozzles

  • 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

 

[![DOI](https://zenodo.org/badge/DOI/10.5281/zenodo.7919600.svg)](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

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Additional details

Related works

Is described by
Journal article: 10.48550/arXiv.2305.07146 (DOI)

Funding

European Commission
ZARATHUSTRA - Revolutionizing advanced electrodeless plasma thrusters for space transportation 950466

References

  • Jimenez et al. (2023). [arXiv:2305.07146]