標題: Titlebook: Mathematical Methods for Objects Reconstruction; From 3D Vision to 3D Emiliano Cristiani,Maurizio Falcone ?,Silvia Tozza Conference proceed [打印本頁] 作者: 拼圖游戲 時間: 2025-3-21 16:30
書目名稱Mathematical Methods for Objects Reconstruction影響因子(影響力)
書目名稱Mathematical Methods for Objects Reconstruction影響因子(影響力)學科排名
書目名稱Mathematical Methods for Objects Reconstruction網(wǎng)絡(luò)公開度
書目名稱Mathematical Methods for Objects Reconstruction網(wǎng)絡(luò)公開度學科排名
書目名稱Mathematical Methods for Objects Reconstruction被引頻次
書目名稱Mathematical Methods for Objects Reconstruction被引頻次學科排名
書目名稱Mathematical Methods for Objects Reconstruction年度引用
書目名稱Mathematical Methods for Objects Reconstruction年度引用學科排名
書目名稱Mathematical Methods for Objects Reconstruction讀者反饋
書目名稱Mathematical Methods for Objects Reconstruction讀者反饋學科排名
作者: meritorious 時間: 2025-3-21 22:28 作者: 游行 時間: 2025-3-22 02:14
Georg Radow,Giuseppe Rodriguez,Ashkan Mansouri Yarahmadi,Michael Breu?tosphere depends on the strength of the plasma source near the surface of the star. We start our analysis with magnetospheric models including pair-production as proposed by Sturrock, Ruderman and Sutherland, and Arons. In the light of these models, all neutron stars observed as pulsars must have re作者: 微粒 時間: 2025-3-22 06:38 作者: radiograph 時間: 2025-3-22 09:45
J. Andreas B?rentzen,Ida Bukh Villesen,Ebba Dellwikysics. However, all conceivable effects predicted by this theory and observable inside our own solar system are largely negligible and could be taken into account by a simple ‘tabulation’ of the correction factors from the traditional Newtonian physics. If these observable effects were found to be s作者: Mitigate 時間: 2025-3-22 16:55
Jesse Beisegel,Johannes Buhl,Rameez Israr,Johannes Schmidt,Markus Bambach,Armin Fügenschuh companion irradiation. Here we discuss the main features of a radiation-driven (RD) evolutionary model that may be applicable to several LMXBs. According to this model, radiation from the accreting compact star in LMXBs ‘vaporizes’ the accretion disk and the companion star by driving a self-sustain作者: agenda 時間: 2025-3-22 19:59
Ashkan Mansouri Yarahmadi,Michael Breu?,Carsten Hartmann,Toni Schneidereitn the general radio pulsar population), and a large fraction (~ 40 percent) of millisecond pulsars are found in binaries..All observational evidence indicates that the millisecond and binary pulsars are relatively old neutron stars that have been spun-up by accretion in binary systems (so-called “re作者: 粗魯?shù)娜?nbsp; 時間: 2025-3-22 21:20
An Overview of Some Mathematical Techniques and Problems Linking 3D Vision to 3D Printing,that they share several mathematical techniques. We try to fill the gap presenting an overview of some techniques for Shape-from-Shading problems as well as for 3D printing with an emphasis on the approaches based on nonlinear partial differential equations and optimization. We also sketch possible 作者: extract 時間: 2025-3-23 05:16
Photometric Stereo with Non-Lambertian Preprocessing and Hayakawa Lighting Estimation for Highly Despecially, the light sources are often unknown and need to be estimated, and the light reflectance is often non-Lambertian. In addition, when approaching the problem to apply photometric techniques at real-world imagery, several parameters appear that need to be fixed in order to obtain high-quality作者: Projection 時間: 2025-3-23 08:21 作者: Negotiate 時間: 2025-3-23 12:39 作者: 偽造 時間: 2025-3-23 16:00
Mixed-Integer Programming Models for Two Metal Additive Manufacturing Methods,ch as sequence optimization. Exact solution techniques for MIPs, most prominently branch-and-cut techniques, have the advantage (compared to heuristics such as genetic algorithms) that they can generate solutions with optimality certificates. The novel process of additive manufacturing opens up a fu作者: somnambulism 時間: 2025-3-23 20:54 作者: Adornment 時間: 2025-3-23 22:52 作者: insightful 時間: 2025-3-24 06:26
Mathematical Methods for Objects Reconstruction978-981-99-0776-2Series ISSN 2281-518X Series E-ISSN 2281-5198 作者: trigger 時間: 2025-3-24 09:51 作者: 得罪 時間: 2025-3-24 14:02 作者: sclera 時間: 2025-3-24 18:13 作者: 昆蟲 時間: 2025-3-24 21:34 作者: resistant 時間: 2025-3-25 01:36 作者: nepotism 時間: 2025-3-25 06:32 作者: 友好關(guān)系 時間: 2025-3-25 08:14
Conference proceedings 2023uture scientific leaders in the field of 3D data acquisition, 3Dscene reconstruction, and 3D printing software development will find an excellent introduction to these problems and to the mathematical techniques necessary to solve them..作者: 豐富 時間: 2025-3-25 12:01 作者: Ligneous 時間: 2025-3-25 18:52
Emiliano Cristiani,Maurizio Falcone,Silvia TozzaeppoSAX added important information on the pulsar emission in the harder band pass whereas EUVE and HST allowed to study neutron stars in the very soft 0.07—0.2 keV and optical/UV bands. More details on results from observations of neutron stars can be found in the Chaps. 6—8. New excellent observat作者: Vertebra 時間: 2025-3-25 20:06
Georg Radow,Giuseppe Rodriguez,Ashkan Mansouri Yarahmadi,Michael Breu?he hot wind equation for the pair plasma and the relativistic Grad-Schlüter-Shafranov (GSS) equation for the magnetic flux function. The structure of the solutions for the hot pair wind equation is discussed. We also show how self-consistent axisymmetric MHD magnetospheres can be constructed by simu作者: 進入 時間: 2025-3-26 03:14
Toby Collins,Adrien Bartoliics and astrophysics of neutron stars and black holes is here attacked from both theoretical and experimental points of view. In the experimental field we range from the reviews and catalogues of galactic X-ray sources (R. Gursky and E. Schreier) and pulsars (E. Groth) to the observations of the opt作者: 六個才偏離 時間: 2025-3-26 06:08 作者: 該得 時間: 2025-3-26 11:05
Jesse Beisegel,Johannes Buhl,Rameez Israr,Johannes Schmidt,Markus Bambach,Armin Fügenschuhlsar can continue to vaporize the low-mass companion star even after the accretion turn-off produced by a strong pulsar wind; (5) the RD-evolutionary model resolves the apparent statistical discrepancy between the number of MSP’s and their LMXB progenitors.作者: 沒有準備 時間: 2025-3-26 16:37 作者: 下垂 時間: 2025-3-26 20:30
2281-518X 3D printing software development will find an excellent introduction to these problems and to the mathematical techniques necessary to solve them..978-981-99-0778-6978-981-99-0776-2Series ISSN 2281-518X Series E-ISSN 2281-5198 作者: Baffle 時間: 2025-3-26 23:00 作者: Institution 時間: 2025-3-27 01:59 作者: 睨視 時間: 2025-3-27 05:50
2281-518X s from highly reputed academic and industrial researchers wi.The volume collects several contributions to the INDAM workshop .Mathematical Methods for Objects Reconstruction.: from 3D Vision to 3D Printing. held in Rome, February, 2021..?The goal of the workshop was to discuss new methods and concep作者: Lumbar-Spine 時間: 2025-3-27 11:02 作者: Embolic-Stroke 時間: 2025-3-27 16:24 作者: flimsy 時間: 2025-3-27 20:41
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