SEISMOSUN

Magnetohydrodynamic Wave Diagnostics of the Solar Atmosphere in the Era of Transformative High-Resolution Observations

 Coordinatore THE UNIVERSITY OF WARWICK 

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 Nazionalità Coordinatore United Kingdom [UK]
 Totale costo 1˙590˙034 €
 EC contributo 1˙590˙034 €
 Programma FP7-IDEAS-ERC
Specific programme: "Ideas" implementing the Seventh Framework Programme of the European Community for research, technological development and demonstration activities (2007 to 2013)
 Code Call ERC-2012-ADG_20120216
 Funding Scheme ERC-AG
 Anno di inizio 2013
 Periodo (anno-mese-giorno) 2013-04-01   -   2018-03-31

 Partecipanti

# participant  country  role  EC contrib. [€] 
1    THE UNIVERSITY OF WARWICK

 Organization address address: Kirby Corner Road - University House -
city: COVENTRY
postcode: CV4 8UW

contact info
Titolo: Ms.
Nome: Catherine
Cognome: Cochrane
Email: send email
Telefono: +44 2476574453

UK (COVENTRY) hostInstitution 1˙590˙034.91
2    THE UNIVERSITY OF WARWICK

 Organization address address: Kirby Corner Road - University House -
city: COVENTRY
postcode: CV4 8UW

contact info
Titolo: Prof.
Nome: Valeri
Cognome: Nakariakov
Email: send email
Telefono: 442477000000
Fax: 442477000000

UK (COVENTRY) hostInstitution 1˙590˙034.91

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 Word cloud

Esplora la "nuvola delle parole (Word Cloud) per avere un'idea di massima del progetto.

space    upon    atmosphere    observables    wave    heating    magnetohydrodynamic    data    solar    phenomena    observational    missions    technique    diagnostics    theoretical    plasma    physics   

 Obiettivo del progetto (Objective)

'Funding is sought for a 5-year project supporting two postdoctoral research assistants and two 4-year PhD studentships to carry out a research programme on qualitative advances of our understanding of basic physical processes operating in the atmosphere of the Sun. This will be accomplished by the use of the unprecedented high-resolution data obtained with the new generation of solar space missions, which allow us to fully implement the novel technique for plasma diagnostics, based upon magnetohydrodynamic waves. The project aims to reveal the mechanisms behind the most intriguing and disturbing solar phenomena: the heating of the corona and the physics of solar flares and mass ejections. The specific objectives are to develop and apply innovative techniques for determining the plasma’s heating function and the characteristic spatial scale of fine structuring; the method for instant diagnostics of plasma parameters by propagating wave trains; the technique for the determination of microphysical processes by macroscopic observables; to discriminate observationally between the theoretically predicted regimes of powerful releases of magnetic energy; to create a theoretical and observational foundation for stellar coronal seismology; and to implement novel methods for the analysis of wave phenomena in spatially-resolved observational data. The project is based upon the synthesis of analytical and numerical theoretical studies and forward modelling of observables, accounting for both magnetohydrodynamic and kinetic effects, and the analysis of multi-wavelength data obtained with space missions SDO, Hinode and STEREO and the Nobeyama radioheliograph. The knowledge to be gained from the project – robust and detailed diagnostics of key parameters and fundamental processes operating in the solar atmosphere – is of vital importance for the creation of models with a predictive value, and for further progression of solar, space and astro plasma physics.'

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