Millimeter and sub-millimeter atmospheric performance at Dome C combining radiosoundings and ATM synthetic spectra
The reliability of astronomical observations at millimeter and sub-millimeter wavelengths closely depends on a low vertical content of water vapor as well as on high atmospheric emission stability. Although Concordia station at Dome C (Antarctica) enjoys good observing conditions in this atmospheric...
Main Authors: | , , , , , , , |
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Format: | Text |
Language: | unknown |
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arXiv
2012
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Subjects: | |
Online Access: | https://dx.doi.org/10.48550/arxiv.1204.0975 https://arxiv.org/abs/1204.0975 |