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- W4652224 abstract "The observations were made at a central wavelength of 580 nm with the UVES red arm and at 437 and 860 nm in dichroic mode, using both the blue and red arms. In one observation block the field has been derotated in order to align the 0.3-arcsec aperture perpendicularly to Venus’s rotation axis, while in other observations it was aligned parallel to it. In each case, spatial information, respectively in the East-West and in the North-South direction, is preserved in the spectra in the direction perpendicular to dispersion, allowing to spatially resolve relative variations in atmospheric rotation." @default.
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- W4652224 date "2010-05-01" @default.
- W4652224 modified "2023-10-11" @default.
- W4652224 title "Characterizing the Venus atmospheric dynamics from ground-based Doppler velocimetry" @default.
- W4652224 hasPublicationYear "2010" @default.
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