Space and Planetary Sciences(P) | ||
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Session Sub-category | Complex & General | |
Session ID | P-CG22 | |
Title | New Developments of Planetary Sciences with ALMA | |
Short Title | Planetary Sciences with ALMA | |
Main Convener | Name | Takayuki Muto |
Affiliation | Division of Liberal Arts, Kogakuin University | |
Co-Convener 1 | Name | Munetake Momose |
Affiliation | The College of Science, Ibaraki University | |
Co-Convener 2 | Name | Hideo Sagawa |
Affiliation | Faculty of Science, Kyoto Sangyo University | |
Co-Convener 3 | Name | Masumi Shimojo |
Affiliation | National Astronomical Observatory of Japan | |
Session Language | JJ | |
Scope | The Atacama Large Millimeter/Submillimeter Array (ALMA) starated its science operation in 2011, and long-baseline observations have become available since 2014. ALMA, with its high sensitivity and resolution, has provided us with qualitatively new information on star and planet formation and small bodies in our Solar System. For example, the discovery of narrow gap structures in the protoplanetary disks around young stars HL Tan and TW Hya enabled us to actually compare the long-standing theoretical models of planet formation with real observations. In our solar system, 60km pixel-scale non-uniform brightness distribution and the rotation of the asteroid Juno are detected. Spatially-resolved thermal mapping of Europa icy surface enables us to search for thermal anomaly in possible plume source regions. As of Cycle 4, Solar observations are available, enabling us, for example, to determine the physical parameters of plasmoid quantitatively. In this session, we overview the latest results of ALMA observations in the field of planetary sciences. We also accept any theoretical and experimental works that are closely related to the observations and discuss the impact on the planetary science community. | |
Presentation Format | Oral and Poster presentation | |
Invited Authors |
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Time | Presentation No | Title | Presenter | Abstract |
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Oral Presentation May 23 AM1 | ||||
09:00 - 09:15 | PCG22-01 | A Spatially Resolved AU-scale Inner Disk around DM Tau with ALMA | Jun Hashimoto | Abstract |
09:15 - 09:30 | PCG22-02 | Possibility to locate the position of the H2O snowline in protoplanetary disks using high-dispersion spectroscopic observations with ALMA | Shota Notsu | Abstract |
09:30 - 09:45 | PCG22-03 | Multiple Paths of Deuterium Fractionation in Protoplanetary Disks | Yuri Aikawa | Abstract |
09:45 - 10:15 | PCG22-04 | ALMA-Hinode-IRIS coordinated observations of solar nanoflares in cycle 4 | Toshifumi Shimizu | Abstract |
10:15 - 10:30 | PCG22-05 | ALMA observations of the solar chromosphere on the polar limb | Takaaki Yokoyama | Abstract |
Oral Presentation May 23 AM2 | ||||
10:45 - 11:00 | PCG22-06 | Absorption and scattering of dust particles in millimeter wavelength | Ryo Tazaki | Abstract |
11:00 - 11:15 | PCG22-07 | Toward understanding origin of gas in debris disks | Aya Higuchi | Abstract |
11:15 - 11:30 | PCG22-08 | Spatial distributions of AlO and SiO molecules around an aluminum-oxide-rich AGB star, W Hydrae | Aki Takigawa | Abstract |
11:30 - 11:45 | PCG22-09 | Spatially Resolved Sub-millimeter Continuum Imaging of Neptune's Upper Troposphere with ALMA: a New Constraint on the Global Atmospheric Circulation | Takahiro IINO | Abstract |
11:45 - 12:00 | PCG22-10 | Toward understanding the origin and habitability of icy bodies in the Solar System with millimeter/sub-millimeter observations | Yasuhito Sekine | Abstract |
Presentation No | Title | Presenter | Abstract |
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Poster Presentation May 23 Core Time | |||
PCG22-P01 | Beam Pattern Modeling of ALMA Single-Dish Antenna and its Deconvolution | Kazumasa Iwai | Abstract |
PCG22-P02 | The development of new solar observing modes of ALMA | Masumi Shimojo | Abstract |
PCG22-P03 | Current status of data analysis of Venusian middle atmosphere observed by ALMA/ Synergy mission with Venus climate orbiter "Akatsuki" | Ryosuke Aoki | Abstract |
PCG22-P04 | Investigation of Venusian upper troposphere using millimeter-wave continuum emission | Hideo Sagawa | Abstract |
PCG22-P05 | On the spatial distribution of Neptune's stratospheric HCN obtained with ALMA | Takahiro IINO | Abstract |
PCG22-P06 | The studies of protoplanetary disks with ALMA: towards comprehensive understanding of planet formation | Munetake Momose | Abstract |
PCG22-P07 | Observations of fresh sublimates in FU Ori disks | Yuri Aikawa | Abstract |
PCG22-P08 | Band 3 continuum and CO molecular line observations towards HD 142527 with ALMA | Soon Kang-Lou | Abstract |
PCG22-P09 | The Flared Gas Structure of the Transitional Disk around Sz 91 | Takashi Tsukagoshi | Abstract |
PCG22-P10 | The Structure of the Asymmetric Multi-Ring Transitional Disk around 2MASS J16394544-2402039 | Mihoko Konishi | Abstract |
PCG22-P11 | The Synthetic ALMA Multiband Analysis of the Dust Properties of the TW Hya Protoplanetary Disk | Seongjoong Kim | Abstract |
PCG22-P12 | ALMA Observations of Dust Emission from Protoplanetary Disks : Comparison with Radial Drift Model of Dust Particles | Hideko Nomura | Abstract |
PCG22-P13 | Detecting Non-Axisymmetric Structures of Protoplanetary Disks from Low-Resolution Radio Interferometric Data | Takayuki Muto | Abstract |
PCG22-P14 | Structure Formation in a Young Protoplanetary Disk by a Magnetic Disk Wind | Sanemichi Takahashi | Abstract |
PCG22-P15 | Origin of gas in debris disks and Ci observation | Hiroshi Kobayashi | Abstract |