SynCOM: A tool for simulating coronal outflows
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arXiv
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| Hauptverfasser: | , , , , |
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| Format: | Preprint |
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2024
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| _version_ | 1866916420470702080 |
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| author | Filho, Valmir Moraes Uritsky, Vadim Thompson, Barbara Gibson, Sarah DeForest, Craig |
| author_facet | Filho, Valmir Moraes Uritsky, Vadim Thompson, Barbara Gibson, Sarah DeForest, Craig |
| contents | SynCOM is a package of procedures written in IDL (Interactive Data Language) that simulates transient solar wind flows. Each function within SynCOM handles specific tasks, such as initializing parameters, generating synthetic profiles, creating Gaussian blobs to represent solar wind features, and producing high-resolution images of the solar corona. This modular design allows users to call or customize individual functions independently, providing flexibility to adjust simulations to different observational or solar wind conditions. The software architecture is designed to facilitate SynCOM, which effectively creates synthetic datasets for testing and verifying feature tracking algorithms. It also takes advantage of the robust capabilities of the IDL for high-performance scientific computing |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2410_01004 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | SynCOM: A tool for simulating coronal outflows Filho, Valmir Moraes Uritsky, Vadim Thompson, Barbara Gibson, Sarah DeForest, Craig Solar and Stellar Astrophysics Instrumentation and Methods for Astrophysics SynCOM is a package of procedures written in IDL (Interactive Data Language) that simulates transient solar wind flows. Each function within SynCOM handles specific tasks, such as initializing parameters, generating synthetic profiles, creating Gaussian blobs to represent solar wind features, and producing high-resolution images of the solar corona. This modular design allows users to call or customize individual functions independently, providing flexibility to adjust simulations to different observational or solar wind conditions. The software architecture is designed to facilitate SynCOM, which effectively creates synthetic datasets for testing and verifying feature tracking algorithms. It also takes advantage of the robust capabilities of the IDL for high-performance scientific computing |
| title | SynCOM: A tool for simulating coronal outflows |
| topic | Solar and Stellar Astrophysics Instrumentation and Methods for Astrophysics |
| url | https://arxiv.org/abs/2410.01004 |