We present laboratory and numerical models investigating the behavioural regimes of rapidly rotating convection in high-latitude planetary core-style settings. Our combined laboratory numerical approach, utilizing simplified geometries, can access more extreme parameters (e.g. Rayleigh numbers Ra <1013; Nusselt numbers Nu <103; Ekman numbers E <3×10−8) than current global-scale dyn…

Tahun Terbit

2003

ISBN/ISSN

979-732-174-6

Deskripsi Fisik

xvii, 241p. ; ill.; 23 cm

No. Panggil

338.04 RIY k