Oral comunication
P. Machado, T. Widemann, J. Peralta, R. Gonçalves, M. Takagi, A. Harutyunyan, Y. J. Lee, G. Gilli, S. Watanabe, T. Satoh, K. Ogohara, A. Yamazaki
Abstract
We will present meridional wind flow results in both Venus hemispheres. We will present, and compare, meridional wind measurements obtained from Akatsuki's space probe (JAXA) observations, namely observations taken with the UVI instrument, and simultaneous coordinated observations obtained with HARPS-N at Telescopio Nazionale Galileo (TNG) in January 2017. We will also compare this new results with meridional wind flow results from previous runs using space-based observations from Venus Express (ESA) with the instrument VIRTIS-M, and groundbased observations at Canada-France-Hawaii Telescope (CFHT) with the high-resolution spectrograph ESPaDOnS (Machado et al. 2014; 2017). Our previous sets of coordinated observations at Venus cloudtops were based in two complementary techniques: Ground-based Doppler velocimetry and cloud-tracked winds using VEx/VIRTIS-M imaging at 0.38 microns.
European Planetary Science Congress 2018
Berlin, Germany
2018 September
