作者: Hans-Jürgen Bolle
DOI: 10.1007/978-94-009-7810-2_18
关键词:
摘要: The physical processes which generate motions in planetary atmospheres are shortly discussed. application of the basic principles is illustrated by (i) relation between thermal structure a atmosphere and its wind system (ii) need for CO2 transports Martian atmosphere. importance radiative observed phenomena can be estimated means scale analysis. An overview given on circulation systems different their possible mechanisms. Finally problem modelling these dynamical stressed.