Space and Planetary Sciences (P)
Session Sub-category Planetary Sciences(PS)
Session ID P-PS04
Title Recent advances in the science of Venus
Short Title Venus science
Main Convener Name Takehiko Satoh
Affiliation Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency
Co-Convener 1 Name George HASHIMOTO
Affiliation Department of Earth Sciences, Okayama University
Co-Convener 2 Name Kevin McGouldrick
Affiliation University of Colorado Boulder
Co-Convener 3 Name Moa Persson
Affiliation Swedish Institute of Space Physics, Uppsala, Sweden
Session Language
E
Scope
Venus, often called as the twin sister planet of the earth, fosters the environment extremely different from that of the earth. Our knowledge about Venus has advanced by ESA's Venus Express and JAXA's Akatsuki missions mostly about its atmosphere (the former is primarily for the chemistry and the latter for the dynamics). Two of the upcoming 3 Venus missions, NASA's VERITAS and ESA's EnVision, are more focused on the geology, interior and evolution of the solid planet, Venus with synthetic aperture radar technique. Another NASA mission DAVINCI sense both the atmosphere and the surface by a descent probe. There may be more to come, such as Chinese VOICE, Indian Shukurayaan-1, Russian Venera-D, and even from a private company (inclined to the astrobiology).

This momentum is supported by the analysis studies with the previous and the current Venus missions, numerical simulations (recently with data assimilation), ground-based observations, laboratory experiments, etc. This session will therefore cover all aspects of science related to Venus, from its interior to the surrounding plasma environment, either by observationally or by theoretically. Implications to the exoplanets are also important objectives of studies of Venus. Contributions by all levels, from early-career researchers to experts, are all welcome.
Presentation Format Oral and Poster presentation
Joint Session with AGU ,EGU
Invited Authors Chizuru Nose (Tohoku University Planetary Plasma and Atmospheric Research Center)
Takeshi Imamura (Graduate School of Frontier Sciences, The University of Tokyo)
KUWAYAMA Shinya (Department of Earth Sciences, Okayama University)
Jorn Helbert (German Aerospace Center)
Hiroki Ando (Kyoto Sangyo University)
Toru Kouyama (National Institute of Advanced Industrial Science and Technology)
Toshiki Matsushima (Kobe University)
Zhuan Guo (the University of Tokyo)
Paul K. Byrne
Time Presentation No Title Presenter
Oral Presentation May 29 PM2
15:30 - 15:45 PPS04-01 Scientific objectives of the AKATSUKI extended mission Atsushi Yamazaki
15:45 - 16:00 PPS04-02 Horizontal structure of Kelvin wave at the Venus cloud top observed by Akatsuki Masataka Imai
16:00 - 16:15 PPS04-03 Retrieval of the Venusian cloud-top sulfur dioxide distribution from Akatsuki UV images Tatsuro Iwanaka
16:15 - 16:30 PPS04-04 Aerosol properties in the Enormous Cloud Cover of Venus as inferred from improved IR2 night-side data Takehiko Satoh
16:30 - 16:45 PPS04-05 Study on the variation of the Venusian polar atmospheric structure and gravity waves using radio occultation data Miyu Sugiura
Oral Presentation May 30 AM1
09:00 - 09:15 PPS04-06 Science objective and status of the EnVision Mission to Venus Jorn Helbert
09:15 - 09:30 PPS04-07 Cross-link radio Occultation measurements of Venus atmosphere by using multiple small satellites Hiroki Ando
09:30 - 09:45 PPS04-08 Phantom: A New Frontiers-class Aerobot Mission to the Venus Skies Paul K. Byrne
09:45 - 10:00 PPS04-09 Rossby wave and its impact on the Venus atmosphere evaluated by observing system simulation experiment Nobumasa Komori
10:00 - 10:15 PPS04-10 The influences of high surface temperature of Venus on its mantle dynamics Masaki Ogawa
Oral Presentation May 30 AM2
10:45 - 11:00 PPS04-11 Role of a Kelvin wave in the formation of Venusian clouds Takeshi Imamura
11:00 - 11:15 PPS04-12 Chemical species and cloud water distributions in the Venus atmosphere calculated by a GCM with chemical and cloud microphysical processes KUWAYAMA Shinya
11:15 - 11:30 PPS04-13 Long-term temperature and thermal-tides variations in upper cloud layer of Venus observed by Akatsuki/LIR Toru Kouyama
11:30 - 11:45 PPS04-14 Ground-based observations of the Venusian O2 airglow emission using WINERED Hideo Sagawa
11:45 - 12:00 PPS04-15 Toward a Mesoscale Dynamics and Microphysical Cloud Model for Venus Kevin McGouldrick
Presentation No Title Presenter
Poster Presentation May 29 PM3
PPS04-P01 Solar wind influence of Venusian hydrogen airglow in thermosphere by Hisaki Chizuru Nose
PPS04-P02 Venusian Ionosphere During Deep Solar Minima (2016-2022): Akatsuki Radio Occulation Observations Keshav R Tripathi
PPS04-P03 Laboratory Study of SO2 Uptake by Sulfuric Acid Droplets in the Venusian Atmospheric Condition Soma Ubukata
PPS04-P04 Ground-based spectral observation of Venus UV absorption by Pirka Telescope Hamamoto Ko
PPS04-P05 Solar phase angle dependence of reflected sunlight obtained from the complete set of Akatsuki IR2 image Takao M. Sato
PPS04-P06 An alternative method to recover the true contrast of Venus' night-side cloud features in Akatsuki/IR2 images Takehiko Satoh
PPS04-P07 Development of Venusian Lightning model for observation of PLD based on JEM-GLIMS measurement of Earth lightning Tatsuharu Ono
PPS04-P08 Superrotation variability and constituent variability at around the cloud-top of Venus Takeshi Horinouchi
PPS04-P09 Characteristics of gravity waves and thermal tides derived from LIR images with radiative transfer modeling Zhuan Guo
PPS04-P10 Toward producing the Venus objective analysis using temperature obtained by Akatsuki Longwave Infrared Camera Yukiko Fujisawa
PPS04-P11 Dynamical and thermodynamical structure in cloud layer simulated by a GCM with correlated-k distribution radiative transfer model Toshiki Matsushima
PPS04-P12 Dependence of the radiative-convective equilibrium structure of the lower atmosphere of Venus on the thermodynamic model Yoshiyuki O. Takahashi