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ST1.6 Amos
www.phase-trans.msm.cam.ac.uk/2006/rotor_Amos_2006.pdf7 Jun 2010: 9, op. cit. 7. S. H. Lalam, H. K. D. H. ... D. H. Bhadeshia, and D. J. C. Mackay, “Estimation of Mechanical Properties of Ferritic Steel Welds, Part 2: Elongation and Charpy toughness,” op. -
IB-descriptors.dvi
mi.eng.cam.ac.uk/~cipolla/lectures/PartIB/old/IB-descriptors.pdf11 May 2010: The way to achieve this robustness is to utilize in-terest points in computing the descriptor as op-posed to the raw image data. -
PowerPoint Presentation
www.phase-trans.msm.cam.ac.uk/2007/C6/New_Crystallography_13.ppt7 Jun 2010: p = OP. closure failure PP’=bt. where bt is total Burgers vector crossing a vector p in interface. -
Equality & Diversity Annual Data Report, 2008/09
https://www.equality.admin.cam.ac.uk/files/data_200809.pdf5 Feb 2010: ff p. op. ula. tio. n. 0%. 10%. 20%. 30%. 40%. -
Evolution and Sustainability of aWildlife Monitoring Sensor Network…
https://mobile-systems.cl.cam.ac.uk/papers/sensys10.pdf1 Sep 2010: this waskey to our success); and the need for continuous interac-tion with domain scientists which allows for unexpected op-timizations. ... are domain scientists that roam through the woods and op-portunistically collect data from storage nodes. -
On wave-action and its relatives
www.damtp.cam.ac.uk/user/mem/andrews-mcintyre-waveac-jfm78.pdf22 Jul 2010: To derive ( 1. 1 ) we follow Sturrock, Whitham and Hayes (op. ... of the whole system, particles as well as disturbance pattern (Peierls, op. -
� � � � � � � � � ...
https://www.dpmms.cam.ac.uk/~ajs1005/ega-index.pdf29 Jan 2010: l m i E n ö X í n í í í Y Ü Ü í í í o Ôp S Õ q â c # 1 ] } # V 2 Ù | Ç r ) < ] -
Demo Abstract: A Shared Sensor Network Infrastructure Christos…
https://mobile-systems.cl.cam.ac.uk/papers/sensys10-demo.pdf30 Aug 2010: In International Conference on Archi-tectural Support for Programming Languages and Op-erating Systems, San Jose, CA, USA, Oct 2002. -
arX iv:1 007. 4517 v1 [ astr o-ph .EP] ...
https://people.ast.cam.ac.uk/~wyatt/bw10.pdf27 Jul 2010: The outcome is summarisedin Fig. 6. 4.4.1 Radiation pressure. Radiation pressure is a radial force which acts in the op-posite direction to the star’s gravity. -
First-order trace formulas for the iterates of theFox–Li operator ...
www.damtp.cam.ac.uk/user/na/NA_papers/NA2010_08.pdf30 Jul 2010: The passage from Wiener–Hopf operators on L2(0,) to Toeplitz op-erators on the Hardy space H2(T) and back can be performed by a standardunitary similarity; see, for example,
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