Mesh Parameterization: Theory and Practice. Global Parameterization and Cone Points Matthias Nieser joint with Felix Kälberer and Konrad Polthier. QuadCover. Curvature lines are intuitive parameter lines. QuadCover : given triangle mesh ) automatically generate global parameterization.

ByPATH PLANNING . Bug Algorithms. Bug1. Bug Algorithms. Bug1. Bug Algorithms. Bug2. Bug Algorithms. Bug2. Bug Algorithms. Bug2. POTENTIAL FUNCTIONS. Potential Field. Attractive – Repulsive Forces. Potential Field. Potential Function. Potential Field. Attractive Potential.

By2003 October-November CMEs. Yang Liu – Stanford University yliu@solar.stanford.edu. Structure and energy of potential field for AR484, 486, and 488. AR: AR0484 TIME: 19:11 UT on 10/23. Energy (potential field): 3.7E+33 ergs. Cube: 300x300x300 arcsec^3. AR: AR0486

ByIR Coronal Tools: Jeff Kuhn Institute for Astronomy, University of Hawaii. Current progress and harmonic convergences IR is good Stokes V is better What’s needed. ATST is coming. The most technologically a dvanced optical and IR “ polarimeter ” ever built.

By12.540 Principles of the Global Positioning System Lecture 04. Prof. Thomas Herring Room 54-820A; 253-5941 tah@mit.edu http://geoweb.mit.edu/~tah/12.540. Review. So far we have looked at measuring coordinates with conventional methods and using gravity field Today lecture:

ByA Diachronic Topological Analysis of the 13th May 2005 Solar Flare. William M.R. Simpson, Angela Des Jardins. University of St. Andrews, Montana State University. Abstract

ByAnother unknown issue of the SW is the origin of slow solar wind. Low-speed wind models. Helmet-streamer. Blob-loop reconnection Wang et al. (1999). Expanding active region Nakagawa & Uchida. Helmet-streamer model. N. Magnetic neutral sheet. S.

ByLecture 6. Obstacle Avoidance. Thanks, Obama!. Funnel Algorithm. Platformer 3. Pathfinding. Pathfinding. Pathfinding is the most common primitive used in game AI A path is a list of instructions for getting from one location to another

ByRevision. Previous lecture consists of: Lagrange’s Generalized Coordinates Lagrange’s Generalized Velocities Generalized Forces Lagrange Equations of Motion for Holonomic Systems. Example: Find the Lagrange equations of motion for a particle moving in a potential field V( x,y,z ) .

ByThe validity of the boundary integral equation for magnetic field extrapolation in open space above spherical surface. He Han, Wang Huaning NAOC, Beijing 2005-07-11. magnetic field extrapolation. Potential field model Force-free field model. field line. Extrapolation scheme:.

ByOrigami and PA design. Common SVD-PXD Meeting. B2GM Nov. 2011. Windmill orientation intensive discussion Drift field Potential field Simulation by Markus Conclusion: Windmill has to be flipped w.r.t. TDR!. Implications on Origami Design. Located at the opposite edge of ladder:

ByPotential Based Routing (PBR) for ICN. Suyong Eum, Kiyohide Nakauchi, Yozo Shoji, Masayuki Murata, Nozomu Nishinaga. 1 st August , 20 12. So which problems are we tackling?. ICN can be considered as a fully distributed caching architecture.

ByNLFFF Solar and Model Results. J.McTiernan NLFFF workshop 5-jun-2006. Optimization method: Wheatland, Roumeliotis & Sturrock, Apj, 540, 1150. Objective: minimize the “Objective Function”. We can write:. If we vary B, such that dB/dt = F, and dB/dt = 0 on the

ByCharles Hermite Center (France). ERSIDP Supélec (France). ParCeL-5/ParSSAP: A Parallel Programming Model and Library for Easy Development and Fast Execution of Simulations of Situated Multi-Agent Systems. SNPD’02. Stéphane Vialle Stephane.Vialle@supelec.fr

ByMobile Sensor Network Deployment Using Potential Fields: A Distributed, Scalable Solution to the Area Coverage Problem. Andrew Howard, Maja J Matari´c, and Gaurav S Sukhatme Speaker : Lee Heon-Jong. Contents. Introduction Related Work Potential Fields Equation of Motion and Control Law

ByPotential Fields Methods Potential Fields A potential field is a field in which the magnitude and direction (vector) of the measurement depends on the location of the measuring instrument.

ByCalibration of Solar Magnetograms and 180 degree ambiguity resolution. Moon, Yong-Jae ( 文 鎔 梓 ) (Korea Astronomy and Space Science Institute). Acknowledgement. 1994 : Huairou, Dr. Ai, Dr. J. Wang, Dr. Zhang 1997 : Mitaka, Dr. Ichimoto, Dr. Sakurai 1999 : M EES , HSP, Dr. Mickey

ByNLFFF Energy Measurement of AR8210. J.McTiernan SSL/UCB. Some Jargon:. Force-free field: JxB = 0, current J is parallel to B Alpha: constant of proportionality, J = α B Linear Force-free field: α is a spatial constant Non-linear Force-free field: α is not constant

ByOn the Extrapolation of the Sun to the Heliosphere. R. A. Howard ACE / SOHO / STEREO / WIND Workshop 8-10 June 2010. Outline. PFSS Modeling Long-term brightness of corona Long-term mass of CMEs Use of HI-type of imaging to see solar wind context. Potential Field Source Surface. PFSS.

ByNLFFF Energy Measurement of AR8210. J.McTiernan SSL/UCB. Some Jargon:. Force-free field: JxB = 0, current J is parallel to B Alpha: constant of proportionality, J = α B Linear Force-free field: α is a spatial constant Non-linear Force-free field: α is not constant

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