Space and Planetary Sciences (P) | ||
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Session Sub-category | Planetary Sciences(PS) | |
Session ID | P-PS05 | |
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 Planetology, Kobe University | |
Co-Convener 2 | Name | Kevin McGouldrick |
Affiliation | University of Colorado Boulder | |
Co-Convener 3 | Name | Silvia Tellmann |
Affiliation | University of Cologne | |
Session Language |
E |
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Scope |
Why Venus and the earth are environmentally so different is a fundamental question of the solar system evolution. Our knowledge about Venus has advanced with 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 body with synthetic aperture radar technique. Another NASA mission DAVINCI will sense both the atmosphere and the surface by a descent probe. More recent moves include: approval of Venus Orbiter Mission (VOM) by the Indian government; upgrading of Chinese VOICE mission to a Venus sample return mission; and the first private sector Venus mission (launch scheduled late 2024). 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. |
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Presentation Format | Oral and Poster presentation | |
Joint Session with | AGU ,EGU | |
Invited Authors |
Takeshi Imamura (Graduate School of Frontier Sciences, The University of Tokyo) Janusz Oschlisniok (Rheinish Institute for Environmental Research, Dep. Planetary Research, Cologne, Germany) Takeshi Horinouchi (Faculty of Environmental Earth Science, Hokkaido University) Takao M. Sato (Hokkaido Information University) Soma Ubukata (Tohoku University) Masataka Imai (The University of Tokyo) |
Time | Presentation No | Title | Presenter |
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Oral Presentation May 27 PM2 | |||
15:30 - 15:45 | PPS05-01 | Image restoration experiment for infrared images of Venus | Zhuan Guo |
15:45 - 16:05 | PPS05-02 | Development of mesoscale structures at the Venusian cloud top | Takeshi Imamura |
16:05 - 16:20 | PPS05-03 | Attempts to improve a Venus' atmospheric chemical model with a focus on temperature | KUWAYAMA Shinya |
16:20 - 16:35 | PPS05-04 | Long-term Studies of the Venusian atmosphere with the Radio Science Experiment VeRa on Venus Express in view of EnVision | Silvia Tellmann |
16:35 - 16:55 | PPS05-05 | Scintillations Observed in Radio Occultation Measurements at Venus | Janusz Oschlisniok |
Oral Presentation May 28 AM1 | |||
9:00 - 9:20 | PPS05-06 | Variability of Venusian cloud-top winds on the order of a hundred Earth days | Takeshi Horinouchi |
9:20 - 9:40 | PPS05-07 | Short-term variation in the dayside cloud top structure of Venus discovered from the complete set of Akatsuki IR2 images | Takao M. Sato |
9:40 - 9:55 | PPS05-08 | Life cycle of large cloud discontinuity in Venus' atmosphere as inferred from Akatsuki/IR2 data | Takehiko Satoh |
9:55 - 10:15 | PPS05-09 | Experimental Study of SO2 Reactive Uptake in Sulfuric Acid Droplets under Venus-analogous Condition | Soma Ubukata |
10:15 - 10:30 | PPS05-10 | Bolide-triggered cloud formation in a planetary atmosphere | Kevin McGouldrick |
Presentation No | Title | Presenter |
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Poster Presentation May 27 PM3 | ||
PPS05-P01 | Development of Model Scattering from Venusian Lightning for observations comparing with JEM-GLIMS measurement of Earth lightning | Tatsuharu Ono |
PPS05-P02 | UV/Visible Spectroscopic Observations of Venus with a Small Ground-based Telescope | Rintaro Eguchi |
PPS05-P03 | Ground-based spectral observation of Venus UV absorption by Pirka Telescope | Hamamoto Ko |
PPS05-P04 | Distributions and Variations of Sulfur Dioxide at the Venusian Cloud Top | Tatsuro Iwanaka |
PPS05-P05 | Variations of Venusian polar atmosphere seen in radio occultation data | Miyu Sugiura |
PPS05-P06 | A Novel Technique for Handling Plasma Asymmetry in Radio Occultation Experiments | Keshav R Tripathi |
PPS05-P07 | Radiative Effects on the Formation of the Stably Stratified Layer in the Lower Atmosphere of Venus | Yoshiyuki O. Takahashi |
PPS05-P08 | Preliminary Steps Toward Data Assimilation Using the Radiation-Coupled AFES-Venus | Toshiki Matsushima |
PPS05-P09 | Validation of data assimilation using Akatsuki LIR observations through observation system simulation experiments on Venus | Yukiko Fujisawa |
PPS05-P10 | Synoptic-scale vortices in the cloud layer on Venus studied by AFES-Venus GCM | Masataka Imai |
PPS05-P11 | A Microphysics Model of Multicomponent Venus' Clouds with a High-Accuracy Condensation Scheme | Hiroki Karyu |