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Finding the Origin of the Slow Solar Wind

Objective

The origins and release mechanisms of stellar winds are long-lasting open challenges in astrophysics. Stellar winds play a fundamental role in the long-term evolution of stars and the habitability of their orbiting planets. In the solar case, the wind is observed in at least two states, fast and slow winds, that differ in their bulk properties and composition, pointing to different coronal origins. A theoretical explanation for the slow wind must explain both its variable bulk properties and its peculiar composition. This includes the measured high charge states of minor ions, the abundance variation of Helium during the solar cycle and the high abundance of elements with low first ionisation potential (so called FIP effect) reaching four times the photospheric abundance. SLOW_SOURCE is a comprehensive research project that will use current and upcoming observations as well as completely novel models of the solar atmosphere to determine the origin of the slow wind. We will develop plasma transport models coupling major and all known important minor constituents along realistic coronal magnetic field lines. This model will be the first of its kind producing modelled observations (spectroscopy, imagery) and expected in situ signatures directly from the modelled minor constituents. Combined with data from space and ground-based observatories, our new multi-species, multi-temperature 3-dimensional modelling of coronal plasma will provide new ways to infer the properties of stellar winds and tools to study the fundamental transport and heating processes of stellar plasmas. Determining the enigmatic release mechanism(s) of the slow solar wind constitutes a key objective of the upcoming Parker Solar Probe mission that will obtain radically new observations right from the start of the project. The project (2019-2024) will also be an excellent preparation for the Solar Orbiter mission that should obtain its first data during the second half of the project (2022-2024).

Fields of science (EuroSciVoc)

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Programme(s)

Multi-annual funding programmes that define the EU’s priorities for research and innovation.

Topic(s)

Calls for proposals are divided into topics. A topic defines a specific subject or area for which applicants can submit proposals. The description of a topic comprises its specific scope and the expected impact of the funded project.

Funding Scheme

Funding scheme (or “Type of Action”) inside a programme with common features. It specifies: the scope of what is funded; the reimbursement rate; specific evaluation criteria to qualify for funding; and the use of simplified forms of costs like lump sums.

ERC-COG - Consolidator Grant

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Call for proposal

Procedure for inviting applicants to submit project proposals, with the aim of receiving EU funding.

(opens in new window) ERC-2018-COG

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Host institution

CENTRE NATIONAL DE LA RECHERCHE SCIENTIFIQUE CNRS
Net EU contribution

Net EU financial contribution. The sum of money that the participant receives, deducted by the EU contribution to its linked third party. It considers the distribution of the EU financial contribution between direct beneficiaries of the project and other types of participants, like third-party participants.

€ 1 937 932,00
Address
RUE MICHEL ANGE 3
75794 PARIS
France

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Region
Ile-de-France Ile-de-France Hauts-de-Seine
Activity type
Research Organisations
Links
Total cost

The total costs incurred by this organisation to participate in the project, including direct and indirect costs. This amount is a subset of the overall project budget.

€ 1 995 902,00

Beneficiaries (2)

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