DRIFT-PHOENIX models

Drift-Phoenix is a computer code that simulates the structure of an atmosphere including the formation of clouds. The code is part of the Phoenix-code family. Drift describes the formation of mineral clouds and allows to predict cloud details, like the size of the cloud particles and their composition.

Identifier
Source https://dc.g-vo.org/rr/q/lp/custom/svo.cab/models/drift
Related Identifier http://svo.cab.inta-csic.es/
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://svo.cab/models/drift
Provenance
Creator Woitke P., Helling C., 2003, A&A, 399, 297
Publisher SVO CAB
Publication Year 2014
OpenAccess true
Contact Enrique Solano, LAEFF Archive Support Team <esm(at)cab.inta-csic.es>
Representation
Resource Type Other; AstroObjects
Version 1.0
Discipline Astrophysics and Astronomy