logo

Unravelling The Structure and Evolution of Solar Magnetic Flux Ropes and Their Magnetosheaths

Sector: Solar • Location: Finland

Source: EU Funding & Tenders Portal

Project
Ended

Coronal Mass Ejections (CMEs) are spectacular stellar eruptions that carry huge amounts of plasma and magnetic flux into the space. The interests in their origin, structure, and dynamics reach from fundamental plasma physics to paramount impact on their parent stars and the surrounding planets. One of the most outstanding problems in the studies of CMEs is the lack of reliable information on their

Status
Closed
Sector
Solar
Location
Finland
Updated
22 Jul 2026
Source
EU Funding & Tenders Portal

ConstructChat

Ask ConstructChat about Unravelling The Structure and Evolution of Solar Magnetic Flux Ropes and Their Magnetosheaths

Pick a question to edit it, or write your own.

First answer free · no account

I am a

Project Information FAQ

Project Information

3 Q
The project “Unravelling The Structure and Evolution of Solar Magnetic Flux Ropes and Their Magnetosheaths” is an infrastructure initiative in the Solar sector, located in Finland. Taiyo aggregates data on it from EU Funding & Tenders Portal.

Participants

Not available for this record.

Status

Original status

ended

Taiyo status

Closed

Taiyo last update

2026-07-22

Contact

Not available for this record.

Description

Description

Coronal Mass Ejections (CMEs) are spectacular stellar eruptions that carry huge amounts of plasma and magnetic flux into the space. The interests in their origin, structure, and dynamics reach from fundamental plasma physics to paramount impact on their parent stars and the surrounding planets. One of the most outstanding problems in the studies of CMEs is the lack of reliable information on their magnetic field properties until observed directly. This severely limits our understanding of many aspects in the lifespan of CMEs and their far-reaching consequences. SolMAG will deliver realistic and detailed information of the magnetic fields in CMEs. We will further use this knowledge to obtain significant breakthroughs in CME research, including unravelling physical processes that control CME initiation and evolution, and characterizing formation and interaction of key CME structures. A unique opportunity is provided by recent advances in data-driven and time-dependent numerical simulations and state-of-the-art high-quality remote-sensing solar observations. We will form an unprecedented synthesis of a revolutionary coupled coronal simulation my group is now developing and innovative cross-scale observational analyses. UH space physics team is exceptionally well-placed to carry out this challenging project: We have an unusually versatile background in CME research and strong experience both in numerical simulations and data analysis covering the whole Sun to Earth chain. SolMAG is also particularly timely now when our society is becoming increasingly dependent on technology that solar eruptions have potential to damage and the role of CMEs influencing planetary and stellar evolution is being emphasized. In addition, this project will be an important contribution to European Space Agency’s activities, including the future Solar Orbiter and BebiColombo missions, which also provides a natural exit strategy for this project.

Location

Country

Finland

Source

Source

EU Funding & Tenders Portal

URL

More Details

Record type

Project

Sector

Solar

Article published date

2026-01-15

More on this project

Research

Free account

View all details

You are reading the public part. A free account opens the rest:

  • Every detail on this project
  • News and media coverage
  • Technical research
View all details

Free account · no card · lands you back on this project