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_images/index_api.svg

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_images/index_contribute.svg

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_images/index_getting_started.svg

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_sources/api/index.rst.txt

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MUSICA API
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==========

_sources/contributing/index.rst.txt

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Contributing
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============
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###############
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Getting Started
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###############
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.. toctree::
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:maxdepth: 1
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:caption: Contents:
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overview
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installation
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Installation
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============
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MUSICA source code may be cloned from its public GitHub repository
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and configured and built with the cmake utility.
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In brief:
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.. code-block:: console
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$ git clone https://github.com/NCAR/musica.git
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$ cd musica
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$ mkdir build
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$ cd build
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$ ccmake ..
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$ make
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$ make install
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Overview
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========
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The specific goal of MUSICA is to produce a new model independent infrastructure,
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which will enable chemistry and aerosols to be simulated
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at a large number of different resolutions in a single, coherent fashion.
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At first, MUSICA will be configured within the NCAR Community Earth system Model (CESM)
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and through this enable full feedbacks between the atmosphere, ocean and land.
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The infrastructure will unify the different chemical transport models
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including CAM-Chem, WACCM and WRF-Chem, and NCAR LES with chemistry
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and a box model in a single modular framework.
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The model infrastructure will be open source,
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flexible and computationally efficient in order
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to facilitate community co-development and use for scientific and operational purposes.
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At the heart of MUSICA is the standalone Model Independent Chemistry Model (MICM), which is a gas-phase kinetic solver. MICM is made available by the MUSICA wrapper which satisfies the requirements of the Common Community Physics Package (CCPP)
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and that can be connected to any CCPP compliant atmosphere model.
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MUSICA and MICM will have a flexible design to handle a variety of gas phase and aerosol schemes
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and associated chemical modules such as deposition or photolysis.

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