Work

Code and data for "Why CMEs Arrive Differently: Solar Cycle Modulation Through Solar Wind Structure"

Year: 2025

Type: software

Abstract: All code and data to reproduce the plots in Gyeltshen et al., 2026, "Why Coronal Mass Ejections Arrive Differently: Solar Cycle Modulation Through Solar Wind Structure", to be published in Space Weather. code/main.py contains script to simulate the CME propagations using HUXt. code/analysis.ipynb contains script to generate plots and perform analysis tests. HUXt model: Mathew Owens, & Luke Barnard. (2024). University-of-Reading-Space-Science/HUXt: HUXT V4.2.0 (v.4.2.0). Zenodo. https://doi.org/10.5281/zenodo.12772120 Not all boundary condition data are uploaded due to storage limit (but are available through the MHDweb modelling website from Predictive Science Inc. https://www.predsci.com/mhdweb/home.php).

Source: Zenodo (CERN European Organization for Nuclear Research)

DOI: 10.5281/zenodo.17750334

Authors: Gyeltshen, Dechen Lhamo, Barnard, Luke, Owens, Mathew

Institution: University of Reading

Language: English

Topic: Solar and Space Plasma Dynamics

Subfield: Astronomy and Astrophysics

Field: Physics and Astronomy

Domain: Physical Sciences

Open Access status: green

Funders: UK Research and Innovation, Natural Environment Research Council, Science and Technology Facilities Council

Awards: Why have space weather forecasts not improved for over a decade?, G2311260295, Was the solar magnetic cycle fundamentally different in the past?, G717687328

OpenAlex ID: W7107957777

Cites:

Cited by: 1

Related to: 10