SPACE PLASMA FLOW

Effect of Inhomogeneous Parallel Flow on Plasma Waves and Instabilities

 Coordinatore LANCASTER UNIVERSITY 

 Organization address address: BAILRIGG
city: LANCASTER
postcode: LA1 4YW

contact info
Titolo: Prof.
Nome: Farideh
Cognome: Honary
Email: send email
Telefono: +44 (0)1524 510402
Fax: -+44 (0)1524 510493

 Nazionalità Coordinatore United Kingdom [UK]
 Totale costo 235˙103 €
 EC contributo 235˙103 €
 Programma FP7-PEOPLE
Specific programme "People" implementing the Seventh Framework Programme of the European Community for research, technological development and demonstration activities (2007 to 2013)
 Code Call FP7-PEOPLE-2007-4-2-IIF
 Funding Scheme MC-IIF
 Anno di inizio 2008
 Periodo (anno-mese-giorno) 2008-12-01   -   2010-11-30

 Partecipanti

# participant  country  role  EC contrib. [€] 
1    LANCASTER UNIVERSITY

 Organization address address: BAILRIGG
city: LANCASTER
postcode: LA1 4YW

contact info
Titolo: Prof.
Nome: Farideh
Cognome: Honary
Email: send email
Telefono: +44 (0)1524 510402
Fax: -+44 (0)1524 510493

UK (LANCASTER) coordinator 0.00

Mappa


 Word cloud

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

parallel    plasma    model    space    theories    instabilities    curvature    flow    hypothesis    realistic    shear    oscillations   

 Obiettivo del progetto (Objective)

'The prevalent theories of parallel flow have considered plasma waves and instabilities in the presence of only flow shear. As a result, these theories have predicted only excitation (destabilization) of instabilities which has lead to the well-known hypothesis that `parallel flow shear is the origin of many space oscillations and instabilities'. However, here we propose to develop a model of space plasma oscillations and instabilities in the presence of a more realistic flow profile including both flow shear and flow curvature. Now, with the inclusion of flow curvature the stability picture is expected to be changed drastically. The flow curvature, contrary to the flow shear, can actually STABILIZE the modes which is rather opposite to the well-know hypothesis of the generation of space fluctuations by the parallel velocity shear. Furthermore, the new model of space oscillations in the presence of both flow shear and curvature, being more realistic, is expected to produce results which should fit better with the spacecraft data. These results are also expected to have important implications in the communication systems and space weather technologies. Apart from the space plasma and fluid dynamics community, the theory proposed to be developed here will also have application in the plasma and fusion energy technology.'

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