Three-dimensional shape distribution of lunar regolith particles collected by the Apollo and Luna programs
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DOI[10.1186/s40623-022-01737-9]to the data of the same series
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- Material Type
- 記事
- Author/Editor
- Akira TsuchiyamaTakashi SakuramaTsukasa Nakano
- Publication, Distribution, etc.
- Publication Date
- 2022-11-26
- Publication Date (W3CDTF)
- 2022-11-26
- Periodical title
- EPS : Earth, Planets and Space
- No. or year of volume/issue
- 74(172)
- Volume
- 74(172)
- ISSN (Periodical Title)
- 1880-5981
- ISSN-L (Periodical Title)
- 1343-8832
- Text Language Code
- eng
- DOI
- 10.1186/s40623-022-01737-9
- Persistent ID (NDL)
- info:ndljp/pid/12685459
- Collection
- Collection (Materials For Handicapped People:1)
- Collection (particular)
- 国立国会図書館デジタルコレクション > 電子書籍・電子雑誌 > その他
- Acquisition Basis
- オンライン資料収集制度
- Date Accepted (W3CDTF)
- 2023-03-07T16:17:02+09:00
- Date Captured (W3CDTF)
- 2023-03-07
- Format (IMT)
- application/pdf
- Access Restrictions
- 国立国会図書館内限定公開
- Service for the Digitized Contents Transmission Service
- 図書館・個人送信対象外
- Availability of remote photoduplication service
- 可
- Periodical Title (URI)
- Periodical Title (Persistent ID (NDL))
- info:ndljp/pid/12287068
- Data Provider (Database)
- 国立国会図書館 : 国立国会図書館デジタルコレクション
- Summary, etc.
- コレクション : 国立国会図書館デジタルコレクション > 電子書籍・電子雑誌 > その他
- DOI
- 10.1186/s40623-022-01737-910.21203/rs.3.rs-1962765/v1
- Related Material
- Additional file 1 of Three-dimensional shape distribution of lunar regolith particles collected by the Apollo and Luna programsThree-dimensional shape distribution of lunar regolith particles collected by the Apollo and Luna programs
- Related Material (URI)
- Is Referenced By
- The influence of chondrules on sub-mm fragment shape distributions in Allende impact experimentsAbrasion experiments of mineral, rock, and meteorite particles: Simulating regolith particles abrasion on airless bodies
- References
- Three‐dimensional microstructure of samples recovered from asteroid 25143 Itokawa: Comparison with LL5 and LL6 chondrite particlesFragment shapes in impact experiments ranging from cratering to catastrophic disruptionInfluence of petrographic textures on the shapes of fine fragments with several tens of microns in impact experiments: comparison with Itokawa regolith particlesThermal fatigue as the origin of regolith on small asteroidsGrain‐scale thermoelastic stresses and spatiotemporal temperature gradients on airless bodies, implications for rock breakdownPebbles and sand on asteroid (162173) Ryugu: In situ observation and particles returned to EarthThree-Dimensional Structure of Hayabusa Samples: Origin and Evolution of Itokawa RegolithThe Importance of Phobos Sample Return for Understanding the Mars-Moon SystemNanomorphology of Itokawa regolith particles: Application to space-weathering processes affecting the Itokawa asteroidExpected shape distribution of asteroids obtained from laboratory impact experimentsFormation and evolution of carbonaceous asteroid Ryugu: Direct evidence from returned samples3D Shape Characterization and Image-Based DEM Simulation of the Lunar Soil Simulant FJS-1The unexpected surface of asteroid (101955) BennuSpace weathering on airless bodiesThree-dimensional study on the interconnection and shape of crystals in a graphic granite by X-ray CT and image analysisAsteroidal catastrophic collisions simulated by hypervelocity impact experimentsCharacterization of Lunar Dust for Toxicological Studies. II: Texture and Shape CharacteristicsShapes of asteroids compared with fragments from hypervelocity impact experimentsX線CTによる岩石内部構造の観察・解析法
- Data Provider (Database)
- 国立情報学研究所 : CiNii Research
- Original Data Provider (Database)
- 雑誌記事索引データベースCrossref科学研究費助成事業データベース科学研究費助成事業データベース科学研究費助成事業データベース学術機関リポジトリデータベースCrossrefCrossref
- Bibliographic ID (NDL)
- 12685459