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Geologic interpretation of the near-infrared images of the surface taken by the Venus Monitoring Camera, Venus Express

MPS-Authors
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Basilevsky,  Alexander T.
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;

/persons/resource/persons104208

Shalygin,  Eugene V.
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;

/persons/resource/persons104248

Titov,  Dmitri V.
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;

/persons/resource/persons104070

Markiewicz,  Wojciech J.
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

/persons/resource/persons103976

Ignatiev,  Nikolay I.
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;

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Citation

Basilevsky, A. T., Shalygin, E. V., Titov, D. V., Markiewicz, W. J., Scholten, F., Roatsch, T., et al. (2012). Geologic interpretation of the near-infrared images of the surface taken by the Venus Monitoring Camera, Venus Express. Icarus, 217(2), 434-450. doi:10.1016/j.icarus.2011.11.003.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0015-082F-3
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