Stellar Turbulent Convection: The Multiscale Nature of the Solar Magnetic Signature

The multiscale dynamics associated with turbulent convection present in physical systems governed by very high Rayleigh numbers still remains a vividly disputed topic in the community of astrophysicists, and in general, among physicists dealing with heat transport by convection. The Sun is a very cl...

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Principais autores:	Stefano Scardigli, Francesco Berrilli, Dario Del Moro, Luca Giovannelli
Format:	Artigo
Jezik:	Inglês
Izdano:	MDPI AG 2021-07-01
Serija:	Atmosphere
Teme:	multiscale convection stellar convection turbulent convection solar convection solar magnetic field solar granulation
Online dostop:	https://www.mdpi.com/2073-4433/12/8/938
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