P23A
Planetary Atmospheres and Their Evolution II Posters

Tuesday, 15 December 2015: 13:40-18:00
Poster Hall (Moscone South)
Primary Conveners:  Feng Tian, Tsinghua University, Beijing, China
Conveners:  Michael H Wong, University of California, Berkeley, CA, United States and David Brain, University of Colorado at Boulder, Boulder, CO, United States
Chairs:  David Brain, University of Colorado at Boulder, Boulder, CO, United States and Michael H Wong, University of California Berkeley, Berkeley, CA, United States
OSPA Liaisons:  Feng Tian, Tsinghua University, Beijing, China
 
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
 
Atmospheric Circulation of Brown Dwarfs and Directly Imaged Extrasolar Giant Planets (71512)
Xianyu Tan and Adam P Showman, University of Arizona, Tucson, AZ, United States
 
Dayside-Nightside Temperature Differences in Hot Jupiter Atmospheres (59538)
Thaddeus David Komacek and Adam P Showman, University of Arizona, Tucson, AZ, United States
 
Three-dimensional Numerical Simulation of Venus' Cloud-level Convection (69263)
Ko-ichiro Sugiyama, Inst Space & Astron Science, JAXA, Kanagawa, Japan, Kensuke Nakajima, Kyushu University, Fukuoka, Japan, Masatsugu Odaka, Hokkaido University, Sapporo, Japan, Takeshi Imamura, JAXA, Kanagawa, Japan and Yoshi-Yuki Hayashi, Kobe University, Kobe, Japan
 
A cyclostrophic transformed Eulerian zonal mean model for the middle atmosphere of slowly rotating planets (75226)
Kaixuan Yao, California Institute of Technology, 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-Lopez1, Ricardo Hueso1, Agustin Sanchez-Lavega2 and Antonio García Muñoz3, (1)University of the Basque Country, Fisica Aplicada I, Donostia, Spain, (2)University of the Basque Country, Donostia, Spain, (3)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)Rheinisches Institut für Umweltforschung, Köln, Germany, (4)Institut für Raumfahrttechnik, Universität der Bundeswehr München, 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)
Hakan Svedhem, ESTEC, Noordwijk, 2201, 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 Sakanoi18, Hiroki Ando26, Shin-ya Murakami6, Takao Sato6, Seiko Takagi27, Kensuke Nakajima23, Javier Peralta6 and Yeon Joo Lee28, (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)The University of Tokyo, 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, 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)ISAS/JAXA, 3-1-1 Yoshinodai/Sag, Japan, (27)Tokai University, Tokyo, Japan, (28)JAXA Japan Aerospace Exploration Agency, Sagamihara, Japan
 
Three-Dimensional Modelling of Venus Photochemistry (72659)
Aurélien Stolzenbach, LATMOS Laboratoire Atmosphères, Milieux, Observations Spatiales, Paris Cedex 05, France
 
Venus Atmospheric Maneuverable Platform (VAMP) - A Low Cost Venus Exploration Concept (81052)
Greg Lee, Northrop Grumman Space Technology, Redondo Beach, CA, United States
 
Pyrite Stability Under Venus Surface Conditions (82708)
Erika Kohler1, Patricia Craig2, Sara Port1, Vincent Chevrier1 and Natasha Johnson3, (1)University of Arkansas, Fayetteville, AR, United States, (2)Lunar and Planetary Institute, Houston, TX, United States, (3)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 Marounina1, Olivier Grasset2, Gabriel Tobie3 and Sabrina Carpy1, (1)LPG, Nantes, France, (2)UMR-CNRS 6112, Nantes, France, (3)University of Nantes, 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 Yung1, (1)California Institute of Technology, Pasadena, CA, United States, (2)Jet Propulsion Laboratory, Pasadena, CA, United States, (3)Rt Solutions Inc., Cambridge, MA, United States, (4)NASA Jet Propulsion Laboratory, Pasadena, 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, David 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
 
Hot Oxygen and Carbon Escape from the Early Atmosphere of Mars (78841)
Ute Amerstorfer1, Hannes Gröller2, Herbert Lichtenegger1, Helmut Lammer1 and Feng Tian3, (1)Space Research Institute, Austrian Academy of Sciences, Graz, Austria, (2)University of Arizona, Tucson, AZ, United States, (3)Tsinghua University, Beijing, China
 
Contrasting Responses to Orbital Precession on Titan and Earth (83688)
Junjun Liu, California Institute of Technology, Pasadena, CA, United States
 
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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