activity
20172020
most citedEquatorial jet in the lower to middle cloud layer of Venus revealed by Akatsuki

41 citations · 115 across the 5 of their papers we have counts for

collaborators

8 papers

astro-ph.EP202025 cited

A Long-lived Sharp Disruption on the Lower Clouds of Venus

J. Peralta, T. Navarro, C. W. Vun +19

Planetary-scale waves are thought to play a role in powering the yet-unexplained atmospheric superrotation of Venus. Puzzlingly, while Kelvin, Rossby and stationary waves manifest…

astro-ph.EP2019

Planetary-scale variations in winds and UV brightness at the Venusian cloud top: Periodicity and temporal evolution

Masataka Imai, Toru Kouyama, Yukihiro Takahashi +9

Planetary-scale waves at the Venusian cloud-top cause periodic variations in both winds and ultraviolet (UV) brightness. While the wave candidates are the 4-day Kelvin wave and 5-d…

astro-ph.EP2019

Long-term variations of Venus' 365-nm albedo observed by Venus Express, Akatsuki, MESSENGER, and Hubble Space Telescope

Yeon Joo Lee, Kandis-Lea Jessup, Santiago Perez-Hoyos +16

An unknown absorber near the cloud top level of Venus generates a broad absorption feature from the ultraviolet (UV) to visible, peaking around 360 nm, and therefore plays a critic…

astro-ph.EP2019

Global structure of thermal tides in the upper cloud layer of Venus revealed by LIR onboard Akatsuki

T. Kouyama, M. Taguchi, T. Fukuhara +11

Longwave Infrared Camera (LIR) onboard Akatsuki first revealed the global structure of the thermal tides in the upper cloud layer of Venus. The data were acquired over three Venusi…

astro-ph.EP20193 cited

Principal Components of Short-term Variability in Venus' UV Albedo

Pushkar Kopparla, Yeon Joo Lee, Takeshi Imamura +1

We explore the dominant modes of variability in the observed albedo at the cloud tops of Venus using the Akatsuki UVI 283-nm and 365-nm observations, which are sensitive to SO2 and…

astro-ph.EP201915 cited

Morphology and dynamics of Venus's middle clouds with Akatsuki/IR1

J. Peralta, N. Iwagami, Sánchez-Lavega +8

The Venusian atmosphere is covered by clouds with super-rotating winds whose accelerating mechanism is still not well understood. The fastest winds, occurring at the cloud tops ($\…