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The effects of space weather extend out across our entire Solar System, but this is a simulation of where everything starts: the sudden, violent, emergence of a \u2018flux rope\u2019 out of the Sun\u2019s magnetic field and into the solar wind. In the process flux ropes may bring along millions of tons of plasma from the solar surface to be released into space, known as a Coronal Mass Ejection, CME.<\/p>\n
This flux rope simulation was produced using one of a suite of models available via ESA\u2019s Virtual Space Weather Modelling Centre, employed by space weather forecasters and researchers.<\/p>\n
This simulation was made using the COCONUT coronal \u2018magnetohydrodynamic\u2019 (MHD) model \u2013 developed by a Katholieke Universiteit Leuven\u00a0team and newly presented in Astronomy and Astrophysics. It simulates the initial moments of a Coronal Mass Ejection (CME) within a realistic MHD representation of the solar corona and wind derived from observed magnetograms, with results matching established CME dynamics.<\/p>\n
CMEs are the largest eruptive processes in our Solar System. They can accelerate outwards at velocities of hundreds of kilometres per second or more. If they line up with Earth then our planet\u2019s magnetic environment is altered in turn, potentially affecting satellites in orbit and power and communications infrastructure on the ground.<\/p>\n
Just like terrestrial weather forecasting, the basis of space weather forecasting is to ingest observation data into detailed software models. The challenge in the case of space weather is that the models have to cover the entire Solar System, starting \u2013 as seen here \u2013 just above the Sun\u2019s surface, into the wider heliosphere and covering CMEs and interactions with the magnetic field of Earth (and other planets).<\/p>\n
\u201cThese are all different models with different physics and different data going in and out of these models,\u201d explains ESA space environment and effects engineer Gregoire Deprez. \u201cThe goal with our Virtual Space Weather Modelling Centre is to have all of them coupled together, working in a chain, accessible through a single web portal. They\u2019re made to run and talk together, with data moving on from one through to the next. We have a whole chain of models that start from the Sun, the solar magnetosphere then propagated down to Earth or your spacecraft of interest.\u201d<\/p>\n
The VSWMC was originally established through ESA\u2019s General Support Technology Programme\u00a0\u2013 readying promising technologies for space and is now supported through the Agency\u2019s Space Safety Programme’s\u00a0Space Weather Office.<\/p>\n
This work has been funded by KU Leuven, Belspo, the EU\u2019s H2020 EUHFORIA 2.0 project and ESA via GSTP (ESA Contract No. 4000133080\/20\/NL\/CRS) which explored integration of full MHD coronal models in which a flux rope CME can be embedded along with other heliospheric modelling.\u00a0<\/p>\n<\/p><\/div>\n<\/p><\/div>\n