Role of ocean heat transport in climates of tidally locked exoplanets around M dwarf stars.
about
Exoplanetary Atmospheres-Chemistry, Formation Conditions, and HabitabilityImportance of ocean salinity for climate and habitability.The importance of planetary rotation period for ocean heat transportThe Habitability of Proxima Centauri b: Environmental States and Observational Discriminants.Exoplanet Biosignatures: Observational Prospects.Exploring the climate of Proxima B with the Met Office Unified Model
P2860
Role of ocean heat transport in climates of tidally locked exoplanets around M dwarf stars.
description
article científic
@ca
article scientifique
@fr
articolo scientifico
@it
artigo científico
@pt
bilimsel makale
@tr
scientific article published on 30 December 2013
@en
vedecký článok
@sk
vetenskaplig artikel
@sv
videnskabelig artikel
@da
vědecký článek
@cs
name
Role of ocean heat transport i ...... oplanets around M dwarf stars.
@en
Role of ocean heat transport i ...... oplanets around M dwarf stars.
@nl
type
label
Role of ocean heat transport i ...... oplanets around M dwarf stars.
@en
Role of ocean heat transport i ...... oplanets around M dwarf stars.
@nl
prefLabel
Role of ocean heat transport i ...... oplanets around M dwarf stars.
@en
Role of ocean heat transport i ...... oplanets around M dwarf stars.
@nl
P2860
P356
P1476
Role of ocean heat transport i ...... oplanets around M dwarf stars.
@en
P2093
P2860
P304
P356
10.1073/PNAS.1315215111
P407
P50
P577
2013-12-30T00:00:00Z