P23A:
Planetary Atmospheres and Their Evolution II Posters


Session ID#: 8694

Session Description:
To understand the nature, the spatial and temporal variabilities, the governing physical processes, and the evolution of planetary atmospheres in and outside our solar system are important contents of planetary sciences and strong driving force of planet exploration/observations. While the long-term evolution of the Earth is constrained by geological and geochemical data, the evolution of other planetary bodies must be reconstructed from planetary mission data and astronomical observations. The discoveries of exoplanets greatly expand the interests of the scientific community on planetary atmospheres and provide a new opportunity for interdisciplinary collaborations between geoscientists, astronomers, and planetary scientists. The session welcomes both observational and theoretical studies relevant to current physical states of planetary atmospheres (including the Earth) and their evolution.
Primary Convener:  Feng Tian, Tsinghua University, Beijing, China
Conveners:  Michael H. Wong, University of California, Berkeley, United States and Dave A Brain, University of Colorado at Boulder, Boulder, CO, United States
Chairs:  Dave A Brain, University of Colorado at Boulder, Boulder, CO, United States and Michael H. Wong, University of California Berkeley, Berkeley, CA, United States
OSPA Liaison:  Feng Tian, Tsinghua University, Beijing, China

Cross-Listed:
  • A - Atmospheric Sciences
Index Terms:

5405 Atmospheres [PLANETARY SCIENCES: SOLID SURFACE PLANETS]
5455 Origin and evolution [PLANETARY SCIENCES: SOLID SURFACE PLANETS]
5704 Atmospheres [PLANETARY SCIENCES: FLUID PLANETS]
6296 Extra-solar planets [PLANETARY SCIENCES: SOLAR SYSTEM OBJECTS]

Abstracts Submitted to this Session:

The depths of clouds on Jupiter: Observational constraints on the O/H ratio (76570)
Michael H. Wong, University of California Berkeley, Berkeley, CA, United States, Gordon L Bjoraker, NASA Goddard Space Flight Center, Greenbelt, MD, United States, Imke De Pater, University of California, Berkeley, Departments of Astronomy and of Earth and Planetary Science, Berkeley, United States and Mate Adamkovics, Clemson University, Department of Physics and Astronomy, Clemson, United States
Atmospheric Circulation of Brown Dwarfs and Directly Imaged Extrasolar Giant Planets (71512)
Xianyu Tan, University of Arizona, Tucson, AZ, United States and Adam P Showman, University of Arizona, Planetary Sciences, Tucson, AZ, United States
Dayside-Nightside Temperature Differences in Hot Jupiter Atmospheres (59538)
Thaddeus David Komacek, University of Arizona, Tucson, United States and Adam P Showman, University of Arizona, Planetary Sciences, Tucson, AZ, United States
Three-dimensional Numerical Simulation of Venus' Cloud-level Convection (69263)
Ko-ichiro Sugiyama1, Kensuke Nakajima2, Masatsugu Odaka3, Takeshi Imamura4, Yoshi-Yuki Hayashi5, Masaki Ishiwatari3 and Takuya Kawabata3,6, (1)Inst Space & Astron Science, JAXA, Kanagawa, Japan, (2)Kyushu University, Fukuoka, Japan, (3)Hokkaido University, Sapporo, Japan, (4)JAXA, Kanagawa, Japan, (5)Kobe University, Kobe, Japan, (6)Tecnos Japan Inc., Tokyo, Japan
A cyclostrophic transformed Eulerian zonal mean model for the middle atmosphere of slowly rotating planets (75226)
Kaixuan Yao1, King-Fai Li2, Cameron Taketa2, Xi Zhang3, Mao-Chang Liang4, Xun Jiang5, Claire E Newman6, Ka-Kit Tung2 and Yuk L Yung7, (1)California Institute of Technology, Pasadena, CA, United States, (2)University of Washington, Department of Applied Mathematics, Seattle, WA, United States, (3)University of California Santa Cruz, Earth and Planetary Sciences, Santa Cruz, CA, United States, (4)Academia Sinica, Institute of Earth Sciences, Taipei, Taiwan, (5)University of Houston, Department of Earth and Atmospheric Sciences, Houston, United States, (6)Aeolis Research, Chandler, United States, (7)California Institute of Technology, Division of Geological and Planetary Sciences, Pasadena, CA, United States
Simulations of Wave Features in Venus' Deep Atmosphere Associated with Topography, Using a Venus GCM (76788)
Helen F Parish, University of California Los Angeles, Los Angeles, CA, United States
Atmospheric dynamics at the southern pole of Venus: Three-dimensional winds, temperature and vorticity (61430)
Itziar Garate-Lopez, University of the Basque Country, Fisica Aplicada I, Donostia, Spain, Ricardo Hueso, Universidad del País Vasco UPV/EHU, Bilbao, Spain, Agustin Sanchez-Lavega, University of the Basque Country, Donostia, Spain and Antonio García Muñoz, Technische Universität Berlin, Berlin, Germany
Context Images for Venus Express Radio Occultations: a Search for a Dynamical-Convective Origin of Cloud-top UV Contrasts (70450)
M Roos-Serote1, Colin F Wilson2, Ryan MacDonald2, Silvia Tellmann3, Bernd Häusler4, Yeon Joo Lee5 and Igor Khatuntsev6, (1)University of Michigan Ann Arbor, Ann Arbor, MI, United States, (2)University of Oxford, Oxford, United Kingdom, (3)University of Cologne; Rheinisches Institut fuer Umweltforschung (RIU), Department of Planetary Research, Cologne, Germany, (4)Bundeswehr University Munich, Institute of Space Technology and Space Applications, Munich, Germany, (5)JAXA Japan Aerospace Exploration Agency, Sagamihara, Japan, (6)Space Research Institute, Moscow, Russia
Venus Upper Atmosphere – Results from the Venus Express Aerobraking Campaign (58800)
Håkan Svedhem, ESTEC, Noordwijk, Netherlands
The result of Venus Orbit Insertion of Akatsuki on December 7th, 2015 (60183)
Masato Nakamura1, Ko-ichiro Sugiyama2, Takeshi Imamura3, Nobuaki Ishii2, Takumi Abe2, Yasuhiro Kawakatsu2, Chikako Hirose2, Takehiko Satoh4, Makoto Suzuki2, Munetaka Ueno5, Atsushi Yamazaki6, Naomoto Iwagami7, Shigeto Watanabe8, Makoto Taguchi9, Tetsuya Fukuhara10, Yukihiro Takahashi8, Manabu Yamada11, Masataka Imai12, Shoko Ohtsuki13, Kazunori Uemizu6, George L Hashimoto14, Masahiro Takagi15, Yoshihisa Matsuda16, Kazunori Ogohara17, Naoki Sato16, Yasumasa Kasaba18, Toru Kouyama19, Naru Hirata20, Ryosuke Nakamura21, Yukio Yamamoto22, Takeshi Horinouchi8, Masaru Yamamoto23, Yoshi-Yuki Hayashi24, Junichi Nakatsuka6, Hiroki Kashimura25, Takeshi Sakanoi26, Hiroki Ando27, Shin-ya Murakami6, Takao Sato6, Seiko Takagi28, Kensuke Nakajima23, Javier Peralta6 and Yeon Joo Lee29, (1)Inst Space & Astron Science, Kanagawa, Japan, (2)Inst Space & Astron Science, JAXA, Kanagawa, Japan, (3)JAXA, Kanagawa, Japan, (4)ISAS/JAXA, Sagamihara-Shi, Japan, (5)ISAS/JAXA, Kanagawa, Japan, (6)ISAS/JAXA, Sagamihara, Kanagawa, Japan, (7)Senshu Univ., Bunkyo-ku, Tokyo, Japan, (8)Hokkaido University, Sapporo, Japan, (9)Rikkyo University, Tokyo, Japan, (10)Hokkaido Univ., Sapporo, Japan, (11)Chiba Institute of Technology, Planetary Exploration Research Center, Narashino, Japan, (12)Graduate School of Hokkaido University, Sapporo, Japan, (13)Senshu University, Kanagawa, Japan, (14)Okayama University, Okayama, Japan, (15)Universiy of Miyazaki, Miyazaki-Gun, Japan, (16)Tokyo Gakugei University, Koganei, Tokyo, Japan, (17)University of Shifa Prefecture, Hikone, Shiga, Japan, (18)Tohoku University, Department of Geophysics, Graduate School of Science, Sendai, Japan, (19)AIST - National Institute of Advanced Industrial Science and Technology, Tsukuba, Japan, (20)University of Aizu, Aizu-Wakamatsu, Japan, (21)National Institute of Advanced Industrial Science and Technology (AIST), Tsukuba, Japan, (22)ISAS Institute of Space and Astronautical Science, Kanagawa, Japan, (23)Kyushu University, Fukuoka, Japan, (24)Kobe University, Kobe, Japan, (25)JAMSTEC, Yokosuka, Kanagawa, Japan, (26)PPARC, Tohoku University, Sendai, Japan, (27)ISAS/JAXA, 3-1-1 Yoshinodai/Sag, Japan, (28)Tokai University, Tokyo, Japan, (29)JAXA Japan Aerospace Exploration Agency, Sagamihara, Japan
Three-Dimensional Modelling of Venus Photochemistry (72659)
Aurélien Stolzenbach, IAA-CSIC, Granada, Spain, Franck Lefèvre, LATMOS Laboratoire Atmosphères, Observations Spatiales, Sorbonne université, UVSQ Université Paris-Saclay, CNRS, Paris, France, Sebastien Lebonnois, CNRS, Paris Cedex 16, France, Anni Elisa Määttänen, LATMOS, UVSQ Paris-Saclay, CNRS, Paris, France, Paris Cedex 05, France and Slimane Bekki, LATMOS Laboratoire Atmosphères, Milieux, Observations Spatiales, Guyancourt, France
Venus Atmospheric Maneuverable Platform (VAMP) - A Low Cost Venus Exploration Concept (81052)
Greg Lee, Ronald S Polidan and Floyd Ross, Northrop Grumman Space Technology, Redondo Beach, CA, United States
Pyrite Stability Under Venus Surface Conditions (82708)
Erika Kohler1, Patricia Craig2, Sara Port3, Vincent F Chevrier3 and Natasha Johnson4, (1)University of Arkansas, Fayetteville, United States, (2)Lunar and Planetary Institute, Houston, TX, United States, (3)University of Arkansas, Fayetteville, AR, United States, (4)NASA Goddard Space Flight Center, Greenbelt, MD, United States
CO2-dominated Atmosphere in Equilibrium with NH3-H2O Ocean: Application to Early Titan and Ocean Planets (61820)
Nadejda Marounina, LPG, Nantes, France, Olivier Grasset, UMR-CNRS 6112, Nantes, France, Gabriel Tobie, University of Nantes, Nantes, France and Sabrina Carpy, Laboratoire de Planétologie et Géodynamique, Nantes, France
Fast and Accurate Radiative Transfer Calculations Using Principal Component Analysis for (Exo-)Planetary Retrieval Models (64934)
Pushkar Kopparla1, Vijay Natraj2, Run-Lie Shia1, Robert J D Spurr3, David Crisp4 and Yuk L Yung5, (1)California Institute of Technology, Pasadena, CA, United States, (2)Jet Propulsion Laboratory, California Institute of Technology, Pasadena, United States, (3)Rt Solutions Inc., Cambridge, MA, United States, (4)NASA Jet Propulsion Laboratory, Pasadena, CA, United States, (5)California Institute of Technology, Division of Geological and Planetary Sciences, Pasadena, CA, United States
Understanding Titan’s Atmospheric Isotope Inventory through Laboratory Photolysis Experiments using Vacuum Ultraviolet Photons from Advanced Light Source Synchrotron (74038)
Subrata Chakraborty, University of California San Diego, La Jolla, CA, United States
Constraining planetary atmospheric density: application of heuristic search algorithms to aerodynamic modeling of impact ejecta trajectories (70526)
Zac Yung-Chun Liu, Arizona State University, Tempe, AZ, United States and Manoochehr Shirzaei, Arizona State University, School of Earth and Space Exploration, Tempe, AZ, United States
Highly Accurate Semi-Empirical IR Line Lists of Asymmetric SO2 Isotopologues: SO18O and SO17O (75540)
Xinchuan Huang1, D Schwenke1 and Timothy J Lee2, (1)NASA Ames Research Center, Moffett Field, CA, United States, (2)NASA Ames Research Ctr, Moffett Field, CA, United States
Pure and N-substituted Small Cyclic Hydrocarbon Cations and Anions Synthesis in The Ionosphere of Titan: An Ab-Initio Quantum Chemical Perspective (75578)
Partha P Bera, NASA - Ames Research Center, Mountain View, CA, United States
Hot Oxygen and Carbon Escape from the Early Atmosphere of Mars (78841)
Ute Amerstorfer1, Hannes Gröller2, Herbert Lichtenegger3, Helmut Lammer3 and Feng Tian4, (1)Austrian Academy of Sciences, Space Research Institute, Vienna, Austria, (2)University of Arizona, Lunar and Planetary Laboratory, Tucson, AZ, United States, (3)Space Research Institute, Austrian Academy of Sciences, Graz, Austria, (4)Tsinghua University, Beijing, China
Contrasting Responses to Orbital Precession on Titan and Earth (83688)
Junjun Liu, California Institute of Technology, Pasadena, CA, United States and Tapio Schneider, ETH Swiss Federal Institute of Technology Zurich, Zurich, Switzerland
History of Water Loss and Atmospheric O2 Buildup on Rocky Exoplanets near M Dwarfs (83838)
Feng Tian, Tsinghua University, Beijing, China

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