Skip to main content
Go to the home page of the European Commission (opens in new window)
English English
CORDIS - EU research results
CORDIS
Content archived on 2024-06-18

Understanding the variability of solar And STellar RAdiative fluxes

Objective

The variable Sun is the primary external driver of natural climate change, as evidenced by positive correlations between solar variability and various climate indicators. Even though the Sun-Earth connection has been under close scrutiny over the last two decades, a number of crucial questions remain open. Thus, in the 4th IPCC assessment report the level of our understanding of the solar influence on climate was graded as very low. One of the reasons for this is our incomplete understanding of solar irradiance variability. In particular, the magnitude (in the UV part of the spectrum) and even the phase (in the visible part of the spectrum) of the solar cycle variation remain highly controversial. Also the magnitude of solar irradiance changes on centennial and longer time scale is uncertain.

The main goal of this project is to incorporate the newest information obtained by the recent high-resolution observations and magnetohydrodynamic (MHD) simulations of the solar atmosphere into SATIRE (Spectral And Total Irradiance Reconstruction), which is one of the most advanced models of solar irradiance variability.  This information will put important constraints on the relationship between the magnetic field strength and the spectral contrasts of solar active regions, crucial for successful modeling of solar irradiance variability. The improved SATIRE model will be employed to compute and release new, more reliable and more physics-based reconstructions of solar total and spectral irradiance over the Holocene. It will also be employed to analyze the unprecedentedly precise photometric time series of Sun-like stars obtained by the Kepler and Corot space missions, whose advent rekindled the interest in solar-stellar comparison. This will allow one to understand whether the photometric variabilities of Sun-like stars are governed by the same physical processes as those acting on the Sun.

Fields of science (EuroSciVoc)

CORDIS classifies projects with EuroSciVoc, a multilingual taxonomy of fields of science, through a semi-automatic process based on NLP techniques. See: The European Science Vocabulary.

You need to log in or register to use this function

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.

Call for proposal

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

FP7-PEOPLE-2013-IEF
See other projects for this call

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.

MC-IEF - Intra-European Fellowships (IEF)

Coordinator

MAX-PLANCK-GESELLSCHAFT ZUR FORDERUNG DER WISSENSCHAFTEN EV
EU contribution
€ 168 794,40
Address
HOFGARTENSTRASSE 8
80539 Munchen
Germany

See on map

Region
Bayern Oberbayern München, Kreisfreie Stadt
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.

No data
My booklet 0 0