標題: Titlebook: Development of a Numerical Simulation Method for Rocky Body Impacts and Theoretical Analysis of Aste; Keisuke Sugiura Book 2020 The Editor [打印本頁] 作者: 補給線 時間: 2025-3-21 18:47
書目名稱Development of a Numerical Simulation Method for Rocky Body Impacts and Theoretical Analysis of Aste影響因子(影響力)
書目名稱Development of a Numerical Simulation Method for Rocky Body Impacts and Theoretical Analysis of Aste影響因子(影響力)學科排名
書目名稱Development of a Numerical Simulation Method for Rocky Body Impacts and Theoretical Analysis of Aste網(wǎng)絡(luò)公開度
書目名稱Development of a Numerical Simulation Method for Rocky Body Impacts and Theoretical Analysis of Aste網(wǎng)絡(luò)公開度學科排名
書目名稱Development of a Numerical Simulation Method for Rocky Body Impacts and Theoretical Analysis of Aste被引頻次
書目名稱Development of a Numerical Simulation Method for Rocky Body Impacts and Theoretical Analysis of Aste被引頻次學科排名
書目名稱Development of a Numerical Simulation Method for Rocky Body Impacts and Theoretical Analysis of Aste年度引用
書目名稱Development of a Numerical Simulation Method for Rocky Body Impacts and Theoretical Analysis of Aste年度引用學科排名
書目名稱Development of a Numerical Simulation Method for Rocky Body Impacts and Theoretical Analysis of Aste讀者反饋
書目名稱Development of a Numerical Simulation Method for Rocky Body Impacts and Theoretical Analysis of Aste讀者反饋學科排名
作者: 胎兒 時間: 2025-3-21 21:11 作者: 雪崩 時間: 2025-3-22 03:25
978-981-15-3724-0The Editor(s) (if applicable) and The Author(s), under exclusive license to Springer Nature Singapor作者: OASIS 時間: 2025-3-22 07:35 作者: Electrolysis 時間: 2025-3-22 10:42
Springer Theseshttp://image.papertrans.cn/d/image/270015.jpg作者: Concomitant 時間: 2025-3-22 16:09 作者: Concomitant 時間: 2025-3-22 19:38
Erbrecht,such numerical simulations, we need knowledge about not only hydrodynamics but also elastic dynamics for intact rocks, fracturing of rocky materials, and friction of completely damaged rocks. In this chapter, we introduce the detailed methods necessary for numerical simulations of asteroidal collisi作者: 有惡意 時間: 2025-3-22 21:29 作者: Arboreal 時間: 2025-3-23 04:49
https://doi.org/10.1007/978-3-662-29974-6acts produce spherical and bilobed shapes but they do not produce flat shapes. The impact velocity is strongly affected by the environments of planetary systems such as the existence of gas components or giant planets. Low-velocity impacts are realized in the primordial environment, while high-veloc作者: recession 時間: 2025-3-23 08:53
https://doi.org/10.1007/978-3-662-29974-6mua was discovered, and its light curve shows that 1I/‘Oumuamua has the size of about 100?m and an extremely elongated shape with the ratio of intermediate to major axis lengths less than 0.3. In this chapter, we introduce results of our simulations that investigate detailed impact conditions to for作者: braggadocio 時間: 2025-3-23 12:05
https://doi.org/10.1007/978-3-662-29974-6 numerical simulations. We also analyzed shapes of actual asteroids and compare them with shapes of impact outcomes produced through our simulations. Finally we applied our simulations to the formation of the extremely elongated shape of 1I/‘Oumuamua. In this chapter, we summarize our study. We also作者: hangdog 時間: 2025-3-23 17:20
Book 2020and have kept their shapes until today. The author also shows that asteroid collisions under certain conditions can produce the extremely elongated shape of an interstellar minor body, 1I/‘Oumuamua. In brief, the book offers a comprehensive investigation of asteroid impacts and shapes, making it a u作者: 合乎習俗 時間: 2025-3-23 18:38
2190-5053 er certain conditions can produce the extremely elongated shape of an interstellar minor body, 1I/‘Oumuamua. In brief, the book offers a comprehensive investigation of asteroid impacts and shapes, making it a u978-981-15-3724-0978-981-15-3722-6Series ISSN 2190-5053 Series E-ISSN 2190-5061 作者: 惰性氣體 時間: 2025-3-23 23:02
Introduction,apter, we introduce the overview of the solar system, the properties of asteroids, the standard solar system formation scenario, and the collisional phenomena between rocky minor bodies as basic knowledge to extract information of the past solar system from asteroids’ shapes.作者: 十字架 時間: 2025-3-24 04:02
Development of a Numerical Simulation Method for Rocky Body Impacts and Theoretical Analysis of Aste作者: Aggrandize 時間: 2025-3-24 07:05 作者: Homocystinuria 時間: 2025-3-24 12:13 作者: 語言學 時間: 2025-3-24 14:50
Method,such numerical simulations, we need knowledge about not only hydrodynamics but also elastic dynamics for intact rocks, fracturing of rocky materials, and friction of completely damaged rocks. In this chapter, we introduce the detailed methods necessary for numerical simulations of asteroidal collisi作者: Fluctuate 時間: 2025-3-24 22:52
Results: Shapes of Impact Outcomes, Database of Asteroid Models from Inversion Techniques provides almost all shapes of known asteroids with diameters larger than 100?km. Thus, in our impact simulations, we set radius of target asteroids to 50?km to allow us to directly compare the results of our simulations with the shapes of actual作者: 形上升才刺激 時間: 2025-3-24 23:42 作者: botany 時間: 2025-3-25 06:07 作者: unstable-angina 時間: 2025-3-25 11:20
Summary and Future Prospects, numerical simulations. We also analyzed shapes of actual asteroids and compare them with shapes of impact outcomes produced through our simulations. Finally we applied our simulations to the formation of the extremely elongated shape of 1I/‘Oumuamua. In this chapter, we summarize our study. We also作者: Arresting 時間: 2025-3-25 13:40 作者: 反感 時間: 2025-3-25 16:25 作者: anchor 時間: 2025-3-25 21:00
2190-5053 pacts, helping readers to develop simulation codes using the.This book describes numerical simulations of collisions between asteroids, based on a unique numerical code developed by the author. The code accurately solves the elastic dynamic equations and describes the effects of fracture and frictio作者: Abominate 時間: 2025-3-26 00:29
https://doi.org/10.1007/978-3-662-29974-6Finally we applied our simulations to the formation of the extremely elongated shape of 1I/‘Oumuamua. In this chapter, we summarize our study. We also state future prospects of our study such as application to other phenomena.作者: FEIGN 時間: 2025-3-26 05:57 作者: GOUGE 時間: 2025-3-26 11:13
Results: Shapes of Impact Outcomes, impact simulations. As a result, we find that similar-mass and low-velocity impacts produce various shapes including extremely flat and elongated shapes. In contrast, high-velocity and destructive impacts mainly produce spherical and bilobed shapes, but they are difficult to produce flat shapes.作者: Fulminate 時間: 2025-3-26 14:43 作者: 入會 時間: 2025-3-26 19:07
https://doi.org/10.1007/978-3-662-29974-6those shapes obtained from several databases, and we find that many flat asteroids are not included in any asteroid families. Both the results of our simulations and the information of actual asteroids suggest that flat shapes of large asteroids are likely to be formed in the primordial environment and they keep their flat shapes until today.作者: 相信 時間: 2025-3-26 21:37
https://doi.org/10.1007/978-3-662-29974-6sing impacting objects larger than 40 degrees. Such low impact velocities are realized in extremely young protoplanetary disks without planetesimals larger than 7?km. Thus, we suggest that 1I/‘Oumuamua came to our solar system from such an extremely young protoplanetary disk.作者: Nebulizer 時間: 2025-3-27 04:45 作者: Hangar 時間: 2025-3-27 07:45 作者: CHAR 時間: 2025-3-27 09:28 作者: 親愛 時間: 2025-3-27 16:58
Leo Gurwitschachtung gerade auf genaue Beibehaltung der Fragestellung und des Erhebungsobjektes geachtet werden mu?. Dies gilt selbst für die noch junge ?Panel?-Methode (s. u.), die ?u?erlich gesehen zwischen Marktuntersuchung und Marktbeobachtung zu stehen scheint.作者: 過時 時間: 2025-3-27 21:34 作者: Isthmus 時間: 2025-3-27 23:52
Ordering Breakfast, Drinks and Snacks,ell extracts, these monoclonal antibodies are mouse immunoglobulins. It is possible that the mouse will recognize antigenic determinants on the human tumor cell not well recognized by the patient’s own immune system.作者: chisel 時間: 2025-3-28 04:04 作者: 館長 時間: 2025-3-28 08:25
Katharina BartschProvides a concise review of support structure optimization in laser powder bed fusion.Includes thermo-mechanical material model of Ti-6Al-4V alloy.Contains cost model for calculation of support-induc
