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Kaiju software includes the Multiscale Atmosphere-Geospace Environment (MAGE) model developed by the Center for Geospace Storms (CGS) as well as other scientific software for simulation of heliospheric environments such as planetary magnetospheres and the solar wind.

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Project Kaiju

Introduction

Kaiju software includes the Multiscale Atmosphere-Geospace Environment (MAGE) model developed by the Center for Geospace Storms (CGS) as well as other scientific software for simulation of heliospheric environments such as planetary magnetospheres and the solar wind.

Current version

Currently supported applications include MAGE (version 1.25) and GAMERA-helio, i.e., the geospace and inner heliosphere applications of the kaiju software. MAGE 1.25 includes GAMERA global magnetosphere model, the RAIJU model of the inner magnetosphere, which is a full rewrite of the Rice Convection Model (RCM), the new energetic precipitation model Dragon King, the REMIX ionospheric electrodynamics module and the TIEGCM model of the ionosphere-thermosphere.

⚠️ Note: The master branch (version 1.25) contains bleeding-edge code that is under active development. If you are an inexperienced user, you might want to stick with more stable MAGE 0.75 and MAGE 1.0 branches.

NASA Community Coordinated Modeling Center (CCMC) availability

Users are also welcome to run previous versions of MAGE via the NASA's Community Coordinated Modeling Center. MAGE versions 0.75 and 1.0 are available for runs on request. MAGE 0.75 includes GAMERA, REMIX and RCM. MAGE 1.0 adds two-way coupling with TIEGCM to MAGE 0.75.

GAMERA-helio is also available for runs on request at the CCMC.

Documentation

Current documentation for the kaiju software is available via Read The Docs.

Analysis

You are encouraged to use the Kaipy package for analysis and visualization of Kaiju simulations.

Rules of the road

All users are strongly encouraged to contact the developers before publication or presentation of MAGE or other Kaiju results. The developers do their best to identify issues and bugs, but make no guarantees. The developers are happy to help the users learn how to apply the model correctly and interpret the results appropriately to ensure their scientific robustness. Additional rules of the road can be found in the Kaiju documentation.

How to cite this work

We ask that the following papers be cited dependent on which configuration the Kaiju software is being run.

For MAGE

For individual model components please cite the following:

GAMERA MHD algorithm and tests: Zhang, B., Sorathia, K.A., Lyon, J.G., Merkin, V.G., Garretson, J.S. and Wiltberger, M., 2019. GAMERA: A three-dimensional finite-volume MHD solver for non-orthogonal curvilinear geometries. The Astrophysical Journal Supplement Series, 244(1), p.20. https://iopscience.iop.org/article/10.3847/1538-4365/ab3a4c/meta.

** GAMERA magnetosphere **: Sorathia, K. A., V. G. Merkin, E. V. Panov, B. Zhang, J. G. Lyon, & J. Garretson, et al. (2020). Ballooning-interchange instability in the near-Earth plasma sheet and auroral beads: Global magnetospheric modeling at the limit of the MHD approximation. Geophysical Research Letters, 47, e2020GL088227. https://doi.org/10.1029/2020GL088227.

REMIX: Merkin, V. G., and J. G. Lyon (2010), Effects of the low-latitude ionospheric boundary condition on the global magnetosphere, J. Geophys. Res., 115, A10202. https://agupubs.onlinelibrary.wiley.com/doi/full/10.1029/2010JA015461.

RAIJU: Team is working on the publication.

Dragon King: Team is working on the publication.

TIEGCM: Qian, L., Burns, A.G., Emery, B.A., Foster, B., Lu, G., Maute, A., Richmond, A.D., Roble, R.G., Solomon, S.C. and Wang, W. (2014). The NCAR TIE-GCM. In Modeling the Ionosphere–Thermosphere System (eds J. Huba, R. Schunk and G. Khazanov). https://doi.org/10.1002/9781118704417.ch7.

For the coupled MAGE model please cite the appropriate component models above and one of the following:

MAGE 0.75: Sorathia, K. A., Michael, A., Merkin, V. G., Ohtani, S., Keesee, A. M., Sciola, A., et al. (2023). Multiscale magnetosphere-ionosphere coupling during stormtime: A case study of the dawnside current wedge. Journal of Geophysical Research: Space Physics, 128, e2023JA031594. https://doi.org/10.1029/2023JA031594.

MAGE 1.0: Pham, K. H., Zhang, B., Sorathia, K., Dang, T., Wang, W., Merkin, V., et al. (2022). Thermospheric density perturbations produced by traveling atmospheric disturbances during August 2005 storm. Journal of Geophysical Research: Space Physics, 127, e2021JA030071. https://doi.org/10.1029/2021JA030071.

MAGE 1.25: Team is working on the publication.

For GAMERA-helio

Provornikova, E., Merkin, V.G., Vourlidas, A., Malanushenko, A., Gibson, S.E., Winter, E. and Arge, C.N., 2024. MHD Modeling of a Geoeffective Interplanetary Coronal Mass Ejection with the Magnetic Topology Informed by In Situ Observations. The Astrophysical Journal, 977(1), p.106. https://iopscience.iop.org/article/10.3847/1538-4357/ad83b1/meta.

Merkin, V. G., J. G. Lyon, D. Lario, C. N. Arge, and C. J. Henney (2016), Time-dependent magnetohydrodynamic simulations of the inner heliosphere, J. Geophys. Res. Space Physics, 121, 2866–2890. https://agupubs.onlinelibrary.wiley.com/doi/10.1002/2015JA022200.

License

Kaiju is distributed under the BSD 3-Clause license.

Contribution guidelines

All contributions should be made by forking this repository and submitting a pull request.

Who do I talk to?

Feel free to send us a message via the feedback form here.

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Kaiju software includes the Multiscale Atmosphere-Geospace Environment (MAGE) model developed by the Center for Geospace Storms (CGS) as well as other scientific software for simulation of heliospheric environments such as planetary magnetospheres and the solar wind.

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