Japan Geoscience Union Meeting 2024

Presentation information

[E] Oral

P (Space and Planetary Sciences ) » P-PS Planetary Sciences

[P-PS04] Recent advances in the science of Venus

Thu. May 30, 2024 10:45 AM - 12:00 PM 101 (International Conference Hall, Makuhari Messe)

convener:Takehiko Satoh(Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency), George HASHIMOTO(Department of Earth Sciences, Okayama University), Kevin McGouldrick(University of Colorado Boulder), Moa Persson(Swedish Institute of Space Physics, Uppsala, Sweden), Chairperson:Takehiko Satoh(Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency), George HASHIMOTO(Department of Earth Sciences, Okayama University)


11:15 AM - 11:30 AM

[PPS04-13] Long-term temperature and thermal-tides variations in upper cloud layer of Venus observed by Akatsuki/LIR

★Invited Papers

*Toru Kouyama1, Masataka Imai2, Takeshi Imamura2, Takeshi Horinouchi3, Shin-ya Murakami4, Yeon Joo Lee5, Makoto Taguchi6 (1.National Institute of Advanced Industrial Science and Technology, 2.University of Tokyo, 3.Hokkaido University, 4.Japan Aerospace Exploration Agency, 5.Institute for Basic Science, 6.Rikkyo University)

Keywords:Venus, Akatsuki, LIR, Thermal tides

While the basic state of Venusian atmosphere (i.e. super-rotation) is stable, it has been recognized that there are lots of variations with various time scales from 4-5 day period to decadal scale in Venusian atmosphere from Venus Express and Akatsuki’s long-term observation. As for the long-term variations, Lee et al (2019) indicated significant variations in UV albedo (more than twice, 20 % to 40 %) and zonal wind speed (more than 30 m s-1) with decadal scale, and Lee et al. (2020) also suggested a 630-day variation in UV albedo. Since these variations have huge amplitudes and are global scale, they should be worth to be considered for understanding global-scale dynamic momentum/material transportation in Venusian atmosphere.
In this study, we focused on long-term temperature data for more than 8 years obtained by Longwave Infrared camera (LIR) onboard Akatsuki to investigate the possible long-term variations. Because long-term temperature data may contain both mean temperature variation and thermal tide variation, which has the largest amplitude in LIR data, we conducted a sliding window analysis by averaging LIR data for more than one Venusian year in terms of local time and latitude that can exclude the thermal-tide component by FFT analysis. From the result, there was a clear quasi-periodical variation in diurnal tide-amplitude in mid-high latitudes whose time scale was 600 – 800 days, while a similar time-scale variation was also confirmed in mean temperature in low-mid latitudes although the amplitude was faint (less than 1 K). Because of the time-scale similarity, the UV albedo variation with a time scale for 630 days might relate these variations.