-
Notifications
You must be signed in to change notification settings - Fork 31
Commit
This commit does not belong to any branch on this repository, and may belong to a fork outside of the repository.
- Loading branch information
Showing
49 changed files
with
1,856 additions
and
1,041 deletions.
There are no files selected for viewing
This file contains bidirectional Unicode text that may be interpreted or compiled differently than what appears below. To review, open the file in an editor that reveals hidden Unicode characters.
Learn more about bidirectional Unicode characters
This file contains bidirectional Unicode text that may be interpreted or compiled differently than what appears below. To review, open the file in an editor that reveals hidden Unicode characters.
Learn more about bidirectional Unicode characters
| Original file line number | Diff line number | Diff line change |
|---|---|---|
| @@ -0,0 +1,13 @@ | ||
| name: Spell Check | ||
|
|
||
| on: [push, pull_request, workflow_dispatch] | ||
|
|
||
| jobs: | ||
| typos-check: | ||
| name: Spell Check with Typos | ||
| runs-on: ubuntu-latest | ||
| steps: | ||
| - name: Checkout Actions Repository | ||
| uses: actions/checkout@v4 | ||
| - name: Check spelling | ||
| uses: crate-ci/[email protected] |
This file contains bidirectional Unicode text that may be interpreted or compiled differently than what appears below. To review, open the file in an editor that reveals hidden Unicode characters.
Learn more about bidirectional Unicode characters
This file contains bidirectional Unicode text that may be interpreted or compiled differently than what appears below. To review, open the file in an editor that reveals hidden Unicode characters.
Learn more about bidirectional Unicode characters
This file contains bidirectional Unicode text that may be interpreted or compiled differently than what appears below. To review, open the file in an editor that reveals hidden Unicode characters.
Learn more about bidirectional Unicode characters
This file contains bidirectional Unicode text that may be interpreted or compiled differently than what appears below. To review, open the file in an editor that reveals hidden Unicode characters.
Learn more about bidirectional Unicode characters
This file contains bidirectional Unicode text that may be interpreted or compiled differently than what appears below. To review, open the file in an editor that reveals hidden Unicode characters.
Learn more about bidirectional Unicode characters
| Original file line number | Diff line number | Diff line change |
|---|---|---|
| @@ -0,0 +1,3 @@ | ||
| [default.extend-words] | ||
| MOR = "MOR" | ||
| dum = "dum" |
This file contains bidirectional Unicode text that may be interpreted or compiled differently than what appears below. To review, open the file in an editor that reveals hidden Unicode characters.
Learn more about bidirectional Unicode characters
| Original file line number | Diff line number | Diff line change |
|---|---|---|
| @@ -0,0 +1,8 @@ | ||
| # GMT 6 Session common arguments shelf | ||
| BEGIN GMT 6.5.0 | ||
| B af WSen | ||
| J X | ||
| JX X15c/0 | ||
| R 0/1/0.1/1 | ||
| @L 1 | ||
| END |
This file contains bidirectional Unicode text that may be interpreted or compiled differently than what appears below. To review, open the file in an editor that reveals hidden Unicode characters.
Learn more about bidirectional Unicode characters
| Original file line number | Diff line number | Diff line change |
|---|---|---|
| @@ -0,0 +1,119 @@ | ||
| --- | ||
| title: 'GeophysicalModelGenerator.jl: A Julia package to visualize geoscientific data and generate model ' | ||
| tags: | ||
| - Julia | ||
| - geosciences | ||
| - geodynamics | ||
| - tectonics | ||
| - geophysics | ||
| authors: | ||
| - name: Boris J.P. Kaus | ||
| orcid: 0000-0002-0247-8660 | ||
| affiliation: 1 # (Multiple affiliations must be quoted) | ||
| - name: Marcel Thielmann | ||
| orcid: 0000-0003-1185-3730 | ||
| affiliation: 2 | ||
| - name: Arne Spang | ||
| orcid: 0000-0002-6107-0403 | ||
| affiliation: 2 | ||
| - name: Luca de Siena | ||
| orcid: 0000-0002-3615-5923 | ||
| affiliation: 3 | ||
| - name: Pascal Aellig | ||
| #orcid: 0000-0003-1185-3730 | ||
| affiliation: 1 | ||
| - name: Jacob Frasukiewicz | ||
| #orcid: 0000-0003-1185-3730 | ||
| affiliation: 1 | ||
| affiliations: | ||
| - name: Johannes Gutenberg University Mainz, Germany | ||
| index: 1 | ||
| - name: University of Bayreuth, Germany | ||
| index: 2 | ||
| - name: Bologna University, Italy | ||
| index: 3 | ||
|
|
||
| date: 27 February 2024 | ||
| bibliography: paper.bib | ||
| --- | ||
|
|
||
| # Summary | ||
|
|
||
| The forces on stars, galaxies, and dark matter under external gravitational | ||
| fields lead to the dynamical evolution of structures in the universe. The orbits | ||
| of these bodies are therefore key to understanding the formation, history, and | ||
| future state of galaxies. The field of "galactic dynamics," which aims to model | ||
| the gravitating components of galaxies to study their structure and evolution, | ||
| is now well-established, commonly taught, and frequently used in astronomy. | ||
| Aside from toy problems and demonstrations, the majority of problems require | ||
| efficient numerical tools, many of which require the same base code (e.g., for | ||
| performing numerical orbit integration). | ||
|
|
||
| # Statement of need | ||
|
|
||
| `Gala` is an Astropy-affiliated Python package for galactic dynamics. Python | ||
| enables wrapping low-level languages (e.g., C) for speed without losing | ||
| flexibility or ease-of-use in the user-interface. The API for `Gala` was | ||
| designed to provide a class-based and user-friendly interface to fast (C or | ||
| Cython-optimized) implementations of common operations such as gravitational | ||
| potential and force evaluation, orbit integration, dynamical transformations, | ||
| and chaos indicators for nonlinear dynamics. `Gala` also relies heavily on and | ||
| interfaces well with the implementations of physical units and astronomical | ||
| coordinate systems in the `Astropy` package [@astropy] (`astropy.units` and | ||
| `astropy.coordinates`). | ||
|
|
||
| `Gala` was designed to be used by both astronomical researchers and by | ||
| students in courses on gravitational dynamics or astronomy. It has already been | ||
| used in a number of scientific publications [@Pearson:2017] and has also been | ||
| used in graduate courses on Galactic dynamics to, e.g., provide interactive | ||
| visualizations of textbook material [@Binney:2008]. The combination of speed, | ||
| design, and support for Astropy functionality in `Gala` will enable exciting | ||
| scientific explorations of forthcoming data releases from the *Gaia* mission | ||
| [@gaia] by students and experts alike. | ||
|
|
||
| # Mathematics | ||
|
|
||
| Single dollars ($) are required for inline mathematics e.g. $f(x) = e^{\pi/x}$ | ||
|
|
||
| Double dollars make self-standing equations: | ||
|
|
||
| $$\Theta(x) = \left\{\begin{array}{l} | ||
| 0\textrm{ if } x < 0\cr | ||
| 1\textrm{ else} | ||
| \end{array}\right.$$ | ||
|
|
||
| You can also use plain \LaTeX for equations | ||
| \begin{equation}\label{eq:fourier} | ||
| \hat f(\omega) = \int_{-\infty}^{\infty} f(x) e^{i\omega x} dx | ||
| \end{equation} | ||
| and refer to \autoref{eq:fourier} from text. | ||
|
|
||
| # Citations | ||
|
|
||
| Citations to entries in paper.bib should be in | ||
| [rMarkdown](http://rmarkdown.rstudio.com/authoring_bibliographies_and_citations.html) | ||
| format. | ||
|
|
||
| If you want to cite a software repository URL (e.g. something on GitHub without a preferred | ||
| citation) then you can do it with the example BibTeX entry below for @fidgit. | ||
|
|
||
| For a quick reference, the following citation commands can be used: | ||
| - `@author:2001` -> "Author et al. (2001)" | ||
| - `[@author:2001]` -> "(Author et al., 2001)" | ||
| - `[@author1:2001; @author2:2001]` -> "(Author1 et al., 2001; Author2 et al., 2002)" | ||
|
|
||
| # Figures | ||
|
|
||
| Figures can be included like this: | ||
|  | ||
| and referenced from text using \autoref{fig:example}. | ||
|
|
||
| Figure sizes can be customized by adding an optional second parameter: | ||
| { width=20% } | ||
|
|
||
| # Acknowledgements | ||
|
|
||
| We acknowledge contributions from Brigitta Sipocz, Syrtis Major, and Semyeong | ||
| Oh, and support from Kathryn Johnston during the genesis of this project. | ||
|
|
||
| # References |
Oops, something went wrong.