Deutsch
 
Benutzerhandbuch Datenschutzhinweis Impressum Kontakt
  DetailsucheBrowse

Datensatz

DATENSATZ AKTIONENEXPORT

Freigegeben

Buchkapitel

DNS of a radiatively driven cloud-top mixing layer as a model for stratocumulus clouds

MPG-Autoren
/persons/resource/persons37131

de Lózar,  Alberto
Max Planck Research Group Turbulent Mixing Processes in the Earth System, The Atmosphere in the Earth System, MPI for Meteorology, Max Planck Society;

/persons/resource/persons37262

Mellado,  Juan-Pedro
Max Planck Research Group Turbulent Mixing Processes in the Earth System, The Atmosphere in the Earth System, MPI for Meteorology, Max Planck Society;

Externe Ressourcen
Es sind keine Externen Ressourcen verfügbar
Volltexte (frei zugänglich)
Es sind keine frei zugänglichen Volltexte verfügbar
Ergänzendes Material (frei zugänglich)
Es sind keine frei zugänglichen Ergänzenden Materialien verfügbar
Zitation

de Lózar, A., & Mellado, J.-P. (2015). DNS of a radiatively driven cloud-top mixing layer as a model for stratocumulus clouds. In J. Fröhlich (Ed.), Direct and Large-Eddy Simulation IX (ERCOFTAC Series; 20) (pp. 419-422). Heidelberg: Springer. doi:10.1007/978-3-319-14448-1_53.


Zitierlink: http://hdl.handle.net/11858/00-001M-0000-002A-5F2C-9
Zusammenfassung
The marine planetary boundary layer topped by stratocumulus clouds (STBL) is key for the planetary radiation balance. In its simplest configuration the STBL consists of a lower moist boundary layer which is topped by a dry and warm free atmosphere. The top of the STBL is populated by stratocumulus clouds that emit long wave radiation, cooling the moist boundary layer. Radiative cooling is thought to be the main source of turbulent energy for the STBL.