English

SynCOM: A tool for simulating coronal outflows

Solar and Stellar Astrophysics 2024-10-03 v1 Instrumentation and Methods for Astrophysics

Abstract

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

Keywords

Cite

@article{arxiv.2410.01004,
  title  = {SynCOM: A tool for simulating coronal outflows},
  author = {Valmir Moraes Filho and Vadim Uritsky and Barbara Thompson and Sarah Gibson and Craig DeForest},
  journal= {arXiv preprint arXiv:2410.01004},
  year   = {2024}
}

Comments

10 pages, 2 figures

R2 v1 2026-06-28T19:04:19.552Z