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Book Chapter

The Martian Atmosphere as a Submillimeter Flux Calibration Source Using an Opaque Molecular Line: Impacts of Temperature Errors Provided by General Circulation Models

MPS-Authors
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Hartogh,  Paul
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;

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Jarchow,  Christopher
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;

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Citation

Kuroda, T., Hartogh, P., & Jarchow, C. (2009). The Martian Atmosphere as a Submillimeter Flux Calibration Source Using an Opaque Molecular Line: Impacts of Temperature Errors Provided by General Circulation Models. In A. Bhardwaj, P. Hartogh, Y. Kasaba, R. Wu, I. Daisuke, & T. Ito (Eds.), Advances in Geosciences (pp. 17-49). World Scientific, Singapore.


Cite as: https://hdl.handle.net/11858/00-001M-0000-0015-0173-5
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