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...

Celý popis

Podrobná bibliografie

Hlavní autoři:	Stefano Scardigli, Francesco Berrilli, Dario Del Moro, Luca Giovannelli
Médium:	Artigo
Jazyk:	Inglês
Vydáno:	MDPI AG 2021-07-01
Edice:	Atmosphere
Témata:	multiscale convection stellar convection turbulent convection solar convection solar magnetic field solar granulation
On-line přístup:	https://www.mdpi.com/2073-4433/12/8/938
Tagy:	Přidat tag Žádné tagy, Buďte první, kdo vytvoří štítek k tomuto záznamu!