Deformation and internal flow of a chondrule-precursor molten sphere in a shocked nebular gas
スポンサーリンク
概要
- 論文の詳細を見る
- Terra Scientific Pub. Co.の論文
- 2003-08-01
著者
-
中本 泰史
東京工業大学地球惑星科学
-
SEKIYA Minoru
Department of Applied Physics, Tokyo Institute of Technology
-
Sekiya Minoru
Department Of Earth And Planetary Sciences Faculty Of Sciences 33 Kyushu University
-
Sekiya Minoru
Department Of Applied Physics Tokyo Institute Of Technology
-
UESUGI Masayuki
Department of Industrial Chemistry, Faculty of Engineering, Nihon University
-
NAKAMOT0 Taishi
Center for Computational Physics, University of Tsukuba
-
NAKAMOTO Taishi
Center for Computational Physics, University of Tsukuba
-
Uesugi Masayuki
Department Of Earth And Planetary Sciences Graduate School Of Sciences 33 Kyushu University
-
SEKIYA Makoto
Department of Physics, Kyoto University
-
SEKIYA Minoru
Department of Physics, Kyoto University
-
SEKIYA Minoru
Department of Earth and Planetary Sciences, Faculty of Sciences 33, Kyushu University
関連論文
- "FIRST"-第一世代天体の起源解明のための専用・汎用計算機融合型クラスタ(HPC-8: 高性能クラスタ)
- 原始太陽系における mm スケールの流体力学(乱流と輸送現象:コーヒーカップから宇宙まで)
- 衝撃波加熱コンドリュール形成 : 形成現場の光学的厚さに関する制限(平成16年度日本惑星科学会最優秀発表賞受賞論文)
- コンドリュール?ショック! : 衝撃波加熱コンドリュール形成モデル
- 非一様宇宙における再電離(基研短期研究会「宇宙における第一世代天体形成」,研究会報告)
- Chapter 12 Settling of Dust Particles and Formation of Planetesimals : Part IV Physical Processes in the Solar Nebula : Origin of the Solar System
- Cosmic-ray exposure age and heliocentric distance of the parent body of H chondrites Yamato-75029 and Tsukuba
- Collisional destruction experiment of chondrules and formation of fragments in the solar nebula
- Formation processes of magnetic spherules collected from deep-sea sediments -Observations and numerical simulations of the orbital evolution-
- 超並列計算機のためのCommodity Networkに基づく並列入出力・可視化システム
- 輻射流体力学による宇宙物理
- The Surface Wave Instability of Stratified Incompressible Cylinders with Differential Rotation : Astrophysics and Relativity
- Numerical Simulation of Viscous Flow by Smoothed Particle Hydrodynamics : Astrophysics and Relativity
- Were planetesimals formed by dust accretion in the solar nebula?
- Solvent Polarities of Supercritical CO_2/Methanol Mixtures
- Dissipation of the Primordial Terrestrial Atmosphere Due to lrradiation of the Solar Far-UV during T Tauri Stage
- Dissipation of the Primordial Terrestrial Atmosphere Due to irradiation of the Solar EUV
- Chapter 23 Gas Capture by Proto-Jupiter and Proto-Saturn : Part VI Growth of the Planets : Origin of the Solar System
- Flow in a Liquid Sphere Moving with a Hypersonic Velocity in a Rarefied Gas : An Analytic Solution of Linearized Equations
- Gravitational Instabilities in a Dust-Gas Layer and Formation of Planetesimals in the Solar Nebula
- Chapter 8 Efficiency of Angular Momentum Transfer by Shear Instability : Part II Formation Processes of Protostars : Origin of the Solar System
- Chapter 7 Stability of the Primordial Solar Nebula : Part II Formation Processes of Protostars : Origin of the Solar System
- Deformation and internal flow of a chondrule-precursor molten sphere in a shocked nebular gas
- Flow in a Liquid Sphere Moving with a Hypersonic Velocity in a Rarefied Gas : An Analytic Solution of Linearized Equations
- Disk-Halo Model for Flat-Spectrum T Tauri Stars
- 多次元輻射輸送計算コードの超並列計算機への実装 : Multiple Wave Front法
- Shear instabilities in the dust layer of the solar nebula II. Different unperturbed states
- Shear instabilities in the dust layer of the solar nebula I. The linear analysis of a non-gravitating one-fluid model without the Coriolis and the solar tidal forces
- On the Peculiarity of the Pion in the Composite Model of Hadrons
- The Generalized Dual Loop Expansion of U(N_c) Gauge Theory
- Shear instabilities in the dust layer of the solar nebula III. Effects of the Coriolis force
- Condition for the formation of the compound chondrules in the solar nebula
- S23-07 原始惑星成長期における微惑星衝撃波による微惑星蒸発(口頭セッション23:原始惑星系円盤,口頭発表)
- 405 A Shock Wave Heating Model for Chondrule Formation
- S33-04P 系外惑星大気による中心星光の屈折と色収差(一般ポスターセッション3,ポスター発表)
- 225 系外惑星大気に入射する光の屈折から生じる現象(オーラルセッション6 観測)
- 320 微惑星衝撃波による微惑星の蒸発(オーラルセッション9 惑星形成過程)
- P106 星雲衝撃波に伴う過飽和珪酸塩ダスト蒸気の生成 : 凝縮物のサイズと形態の多様性(ポスター:一般,ポスターセッション1)
- 402 原始太陽系星雲中衝撃波によるコンドリュール形成 : コンパウンド・コンドリュールの形成(セッション4)
- Thermal evolution of icy planetesimals in the solar nebula