磁気流体力学シミュレーションを用いた原始惑星系円盤の乱流・熱構造の理解

Notes on use

Search by Bookstore

This page shows libraries in Japan other than the National Diet Library that hold the material.

Please contact your local library for information on how to use materials or whether it is possible to request materials from the holding libraries.

other

Tokyo Tech Research Repository
Digital
You can check the holdings of institutions and databases with which Institutional Repositories DataBase(IRDB)(Institutional Repository) is linked at the site of Institutional Repositories DataBase(IRDB)(Institutional Repository).
Tokyo Tech Research Repository

You can check the details of this material, its authority (keywords that refer to materials on the same subject, author's name, etc.), etc.

Material Type: 博士論文
Title: 磁気流体力学シミュレーションを用いた原始惑星系円盤の乱流・熱構造の理解
Author/Editor: 森, 昇志
Mori, Shoji
Author Heading: 森, 昇志
Mori, Shoji
Publication Date: 2019-03
Publication Date (W3CDTF): 2019-03
Alternative Title: Understanding the turbulent and thermal structure of protoplanetary disks with magnetohydrodynamic simulations
Degree grantor/type: 東京工業大学
Date Granted: 2019-03-26
Dissertation Number: 甲第11059号
Degree Type: 博士(理学)
Text Language Code: eng
Subject Heading: 惑星形成
Planet formation
原始惑星系円盤
Protoplanetary disk
磁気流体力学
Magnetohydro dynamics
Target Audience: 一般
Note (General): identifier:oai:t2r2.star.titech.ac.jp:50461347
Format (IMT): application/pdf
Source: http://t2r2.star.titech.ac.jp/rrws/file/CTT100788621/ATD100000413/thesis_16D00470_森昇志.pdf （fulltext）
http://t2r2.star.titech.ac.jp/rrws/file/CTT100788621/ATD100000413/thesis_16D00470_%E6%A3%AE%E6%98%87%E5%BF%97.pdf
Access Restrictions: インターネット公開
Data Provider (Database): 国立情報学研究所 : 学術機関リポジトリデータベース（IRDB）（機関リポジトリ）
https://irdb.nii.ac.jp
Original Data Provider (Database): 東京工業大学 : 東京工業大学リサーチリポジトリ