Space and Planetary Sciences (P) | ||
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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. |
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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 |
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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 |
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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 |