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| 1 | +[](https://ray-chew.github.io/spec_appx/index.html) |
| 2 | + |
| 3 | +<h2 align="center">Constrained Spectral Approximation Method</h2> |
| 4 | + |
| 5 | + |
| 6 | +<p align="center"> |
| 7 | +<a href="https://github.com/ray-chew/spec_appx/actions/workflows/documentation.yml"> |
| 8 | +<img alt="GitHub Actions: docs" src=https://github.com/ray-chew/spec_appx/actions/workflows/documentation.yml/badge.svg> |
| 9 | +</a> |
| 10 | +<a href="https://www.gnu.org/licenses/agpl-3.0"> |
| 11 | +<img alt="License: GNU GPL v3" src=https://img.shields.io/badge/License-AGPL_v3-blue.svg> |
| 12 | +</a> |
| 13 | +<a href="https://github.com/psf/black"> |
| 14 | +<img alt="Code style: black" src=https://img.shields.io/badge/code%20style-black-000000.svg> |
| 15 | +</a> |
| 16 | +</p> |
| 17 | + |
| 18 | + |
| 19 | +The Constrained Spectral Approximation Method (CSAM) is a physically sound and robust method for approximating the spectrum of subgrid-scale orography. It operates under the following constraints: |
| 20 | + |
| 21 | +* Utilises a limited number of spectral modes (no more than 100) |
| 22 | +* Significantly reduces the complexity of physical terrain by over 500 times |
| 23 | +* Maintains the integrity of physical information to a large extent |
| 24 | +* Compatible with unstructured geodesic grids |
| 25 | +* Inherently scale-aware |
| 26 | + |
| 27 | +This method is primarily used to represent terrain for weather forecasting purposes, but it also shows promise for broader data analysis applications. |
| 28 | + |
| 29 | +--- |
| 30 | + |
| 31 | +**[Read the documentation here.](https://ray-chew.github.io/spec_appx/index.html)** |
| 32 | + |
| 33 | +--- |
| 34 | + |
| 35 | +## Requirements |
| 36 | + |
| 37 | +See [`requirements.txt`](https://github.com/ray-chew/spec_appx/blob/main/requirements.txt) |
| 38 | + |
| 39 | +> **NOTE:** The Sphinx dependencies can be found in [`docs/conf.py`](https://github.com/ray-chew/spec_appx/blob/main/docs/source/conf.py). |
| 40 | +
|
| 41 | + |
| 42 | +## Usage |
| 43 | + |
| 44 | +### Installation |
| 45 | + |
| 46 | +Make a fork and clone your remote forked repository. |
| 47 | + |
| 48 | +### Configuration |
| 49 | + |
| 50 | +The user-defined input parameters are in the [`inputs`](https://github.com/ray-chew/spec_appx/tree/main/inputs) subpackage. These parameters are imported into the run scripts in [`runs`](https://github.com/ray-chew/spec_appx/tree/main/runs). |
| 51 | + |
| 52 | +### Execution |
| 53 | + |
| 54 | +A simple setup can be found in [`runs.idealised_isosceles`](https://github.com/ray-chew/spec_appx/blob/main/runs/idealised_isosceles.py). To execute this run script: |
| 55 | + |
| 56 | +```console |
| 57 | +python3 ./runs/idealised_isosceles.py |
| 58 | +``` |
| 59 | + |
| 60 | +However, the codebase is structured such that the user can easily assemble a run script to define their own experiments. Refer to the documentation for the available APIs. |
| 61 | + |
| 62 | +## License |
| 63 | + |
| 64 | +GNU GPL v3 (tentative) |
| 65 | + |
| 66 | +## Contributions |
| 67 | + |
| 68 | +Refer to the open issues that require attention. |
| 69 | + |
| 70 | +Any changes, improvements, or bug fixes can be submitted to upstream via a pull request. |
| 71 | + |
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