The data products derived and presented in the manuscript of "Planetary-scale variations in winds and UV brightness at the Venusian cloud top: Periodicity and temporal evolution" to Journal of Geophysical Research - Planets. All original Akatsuki/UVI images are available via Data ARchives and Transmission System (DARTS, https://darts.isas.jaxa.jp/planet/project/akatsuki/), provided by Center for Science-satellite Operation and Data Archive (C-SODA) at ISAS/JAXA, and NASA PDS Atmospheres Node. The detailed cloud-tracking methodology is given by Ikegawa and Horinouchi (2016), Horinouchi et al. (2017), and Horinouchi et al. (2018)
A cloud opacity contrast feature that has been called a “long-lived sharp disruption” has been seen ...
International audienceAn unknown absorber near the cloud-top level of Venus generates a broad absorp...
The files contain the time series of the longitudinal gradient of Venusian cloud's brightness temper...
The data products derived and presented in the manuscript of "Planetary-scale variations in winds an...
International audienceWe present new wind velocities and its variability at Venus cloud-tops (≈70 km...
We present joint analysis of the UV (365 nm) images captured by the cameras on board ESA’s Venus Exp...
The dataset for publication "Twelve years cycle in the cloud top winds derived from VMC/Venus E...
Abstract Venus is covered with thick clouds. Ultraviolet (UV) images at 0.3–0.4 microns show detaile...
The dataset contain the derived cloud motions from Akatsuki LIR level3c and the corrected LIR level3...
To date dynamical observations of the Venus clouds have delivered mainly either only short-term or l...
More than three decades have passed since the publication of the last review of the Venus clouds and...
Abstract We provide an overview of data products from observations by the Japanese Venus Climate Orb...
International audienceA fast equatorial jet in the Venusian cloud layer has been revealed by the Aka...
This is the derived data, presented in a publication entitled "Spatial and temporal variability of t...
An unknown absorber near the cloud-top level of Venus generates a broad absorption feature from the ...
A cloud opacity contrast feature that has been called a “long-lived sharp disruption” has been seen ...
International audienceAn unknown absorber near the cloud-top level of Venus generates a broad absorp...
The files contain the time series of the longitudinal gradient of Venusian cloud's brightness temper...
The data products derived and presented in the manuscript of "Planetary-scale variations in winds an...
International audienceWe present new wind velocities and its variability at Venus cloud-tops (≈70 km...
We present joint analysis of the UV (365 nm) images captured by the cameras on board ESA’s Venus Exp...
The dataset for publication "Twelve years cycle in the cloud top winds derived from VMC/Venus E...
Abstract Venus is covered with thick clouds. Ultraviolet (UV) images at 0.3–0.4 microns show detaile...
The dataset contain the derived cloud motions from Akatsuki LIR level3c and the corrected LIR level3...
To date dynamical observations of the Venus clouds have delivered mainly either only short-term or l...
More than three decades have passed since the publication of the last review of the Venus clouds and...
Abstract We provide an overview of data products from observations by the Japanese Venus Climate Orb...
International audienceA fast equatorial jet in the Venusian cloud layer has been revealed by the Aka...
This is the derived data, presented in a publication entitled "Spatial and temporal variability of t...
An unknown absorber near the cloud-top level of Venus generates a broad absorption feature from the ...
A cloud opacity contrast feature that has been called a “long-lived sharp disruption” has been seen ...
International audienceAn unknown absorber near the cloud-top level of Venus generates a broad absorp...
The files contain the time series of the longitudinal gradient of Venusian cloud's brightness temper...