Titlebook: Mathematical Methods for Objects Reconstruction; From 3D Vision to 3D Emiliano Cristiani,Maurizio Falcone †,Silvia Tozza Conference proceed

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书目名称Mathematical Methods for Objects Reconstruction影响因子(影响力)




书目名称Mathematical Methods for Objects Reconstruction影响因子(影响力)学科排名




书目名称Mathematical Methods for Objects Reconstruction网络公开度




书目名称Mathematical Methods for Objects Reconstruction网络公开度学科排名




书目名称Mathematical Methods for Objects Reconstruction被引频次




书目名称Mathematical Methods for Objects Reconstruction被引频次学科排名




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书目名称Mathematical Methods for Objects Reconstruction年度引用学科排名




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书目名称Mathematical Methods for Objects Reconstruction读者反馈学科排名

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Georg Radow,Giuseppe Rodriguez,Ashkan Mansouri Yarahmadi,Michael Breußtosphere 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

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J. Andreas Bærentzen,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

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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

agenda

Ashkan Mansouri Yarahmadi,Michael Breuß,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

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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

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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

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