activity
20172022
most citedGlobal structure of thermal tides in the upper cloud layer of Venus revealed by LIR onboard Akatsuki

46 citations · 255 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.EP2022

Reflectivity of Venus' dayside disk during the 2020 observation campaign: outcomes and future perspectives

Yeon Joo Lee, Antonio García Muñoz, Atsushi Yamazaki +28

We performed a unique Venus observation campaign to measure the disk brightness of Venus over a broad range of wavelengths in August and September 2020. The primary goal of the cam…

astro-ph.EP2020★ 14 cited

Brightness modulations of our nearest terrestrial planet Venus reveal atmospheric super-rotation rather than surface features

Y. J. Lee, A. García Muñoz, T. Imamura +4

Terrestrial exoplanets orbiting within or near their host stars' habitable zone are potentially apt for life. It has been proposed that time-series measurements of reflected starli…

astro-ph.EP2020★ 25 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★ 34 cited

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★ 26 cited

New cloud morphologies discovered on the Venus's night during Akatsuki

J. Peralta, A. Sánchez-Lavega, T. Horinouchi +8

During the years 2016 to 2018, the instruments Akatsuki/IR2 (JAXA) and IRTF/SpeX (NASA) acquired a large set of images at 1.74, 2.26 and 2.32 μm to study the nightside mid-to-lower…

astro-ph.EP2019★ 46 cited

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.EP2017★ 31 cited

Return to Venus of the Japanese Venus Climate Orbiter AKATSUKI

Masato Nakamura, Yasuhiro Kawakatsu, Chikako Hirose +19

Japanese Venus Climate Orbiter/AKATSUKI was proposed in 2001 with strong support by international Venus science community and approved as an ISAS (The Institute of Space and Astron…

astro-ph.EP2017★ 41 cited

Equatorial jet in the lower to middle cloud layer of Venus revealed by Akatsuki

T. Horinouchi, S. Murakami, T. Satoh +15

The Venusian atmosphere is in a state of superrotation where prevailing westward winds move much faster than the planet's rotation. Venus is covered with thick clouds that extend f…

astro-ph.EP2017★ 38 cited

Stationary waves and slowly moving features in the night upper clouds of Venus

J. Peralta, R. Hueso, A. Sánchez-Lavega +9

At the cloud top level of Venus (65-70 km altitude) the atmosphere rotates 60 times faster than the underlying surface, a phenomenon known as superrotation. Whereas on Venus's days…