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Methodology for estimating the magnetic Prandtl number and application to solar surface small-scale dynamo simulations

Informazioni aggiuntive

Tipo
Contributo in atti di conferenza
Anno
2021
Lingua
Inglese
Abstract
Context. A crucial step in the numerical investigation of small-scale dynamos in the solar atmosphere consists of an accurate determination of the magnetic Prandtl number, Prm, stemming from radiative magneto-hydrodynamic (MHD) simulation
Atti di conferenza
16th European Solar Physics Meeting (ESPM-16)
Parole chiave
irsol-posters