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Proc. Nail. Acad. Sci. USAVol. 89, pp. 20-22, January ...
www.damtp.cam.ac.uk/user/gold/pdfs/teaching/ufk_papers/proteins/levinthal.pdf4 Oct 2010: 20. The publication costs of this article were defrayed in part by page chargepayment. ... 10-20. UlkT1. 1] FIG. 1. Mean first-passage time, in years, as a function of theenergy bias U/kT. -
www.damtp.cam.ac.uk/user/sje30/teaching/r/Rfiles/ChlorellaGrowth.txt
www.damtp.cam.ac.uk/user/sje30/teaching/r/Rfiles/ChlorellaGrowth.txt6 Oct 2010: # light level, Chlorella maximum growth rate 20 1.73 20 1.65 20 2.02 20 1.89 21 2.61 24 1.36 44 2.37 60 2.08 90 -
Solar Plasma Spectroscopy: Achievements and Future Challenges
www.damtp.cam.ac.uk/user/astro/conference_web/accommodation.html4 Aug 2010: Edmund's College at 45.00 GBP per night including breakfast. 20 standard rooms are available in Churchill College at 30.00 GBP per night including breakfast. -
Explaining the flow of elastic liquids
www.damtp.cam.ac.uk/user/hinch/talks/APS2010.pdf18 Nov 2010: a. 1e-05. 0.0001. 0.001. 0.01. 0 5 10 15 20. t. ... 35. FENE capillary squeezing. Filament breaks in with FENE L = 20. -
Programme - Conservation Areas Seminar - 8 June - issued
www.damtp.cam.ac.uk/user/pvl/26.6.10.pdf11 Jun 2010: Or bring your own lunch. Other lunch opportunities – 15-20 min walk to historic city centre or use Park & Ride bus. ... He has worked for Cambridge City Council for nearly 20 years, and now manages the conservation and tree teams. -
Les liquides \351lastiques: si courants et pourtant si bizarres
www.damtp.cam.ac.uk/user/hinch/talks/GrandPublic.pdf11 Jan 2010: Exemple: pour manger. a. 1e-05. 0.0001. 0.001. 0.01. 0 5 10 15 20. ... Un petit peu de théorie. Les liquides élastiques. Bien étudiés depuis 20 ans? -
A load of balls in Newton's cradle - or Fragmentation of a line…
www.damtp.cam.ac.uk/user/hinch/talks/YRM2010.pdf26 Mar 2010: Chain of 25 particle, 20 rebound. ẋn(). 0.01. 0.1. 1 10. ... But why n3/4? Not diffusion. Rebound velocities. Chain of 25 particle, 20 rebound. -
Lect01.dvi
www.damtp.cam.ac.uk/user/na/PartIB/Lect01.pdf12 Jan 2010: 4.75 4.0 102 7.3 1010. Table: Errors for n = 20. -
Tall Buildings in Cambridge: what do YOU think?An evening ...
www.damtp.cam.ac.uk/user/pvl/TALL/3.3.10_programme.pdf23 Feb 2010: Professor Peter Carolin. (Chair, City’s Design & Conservation Panel)19.20 Economic & environmental sustainability – Ian Gilder (Environmental Resource. ... Management)19.35 Density and quality – Sir Richard MacCormac (MJP Architects)19.50 Questions -
PowerPoint Presentation
www.damtp.cam.ac.uk/user/astro/conference_web/talks/Bradshaw_Mason2010.pdf22 Nov 2010: Strongest signature at 20 s Fe XII (1.6 MK) and Fe XIII (1.6 MK). ... Ongoing – Initial Results. Run 14: Peak temperature = 20 MK Hot emission makes negligible contribution to 94,. -
metricity-final.dvi
www.damtp.cam.ac.uk/user/md327/JDG_published.pdf27 Jan 2010: 3.20) V Ψ :=. 6. p=1. VpΨp = 0,. where. Ψ = (ψ1,ψ2,ψ3,µ,ν,ρ)T. ... 2/3 [6, 20].The zero set of this section intersects each rational curve in Z at twopoints. -
SOXS-Cambridge
www.damtp.cam.ac.uk/user/astro/conference_web/talks/Jain_Mason2010.pdf22 Nov 2010: 7. Flux ratio of Fe to Fe/Ni line features decreases exponentially with flare plasma temperature in 12-20 MK. ... non-thermal. Any non-thermal contribution to line formation? • “The >20 keV electrons contain 10 to 50% of the total energy output”. -
Statistical Physics Matthew Wingate∗ 26 January 2010 ∗Comment &…
www.damtp.cam.ac.uk/user/wingate/Notes/StatPhys/thermo.pdf26 Jan 2010: Quantitiesthat remain unchanged under scale transformations are called intensive. 3 THERMODYNAMICS FROM STATISTICAL MECHANICS 20. -
Slide 1
www.damtp.cam.ac.uk/user/astro/conference_web/talks/Liang_poster.pdf22 Nov 2010: 12 16 20 24 28 32 360.00. 0.05. 0.10. 0.15. 0.20. ... 15+ 16+ 17+ 18+ 19+ 20+ 21+ 22+ 23+ 24+ 25+ 26+ 27+ 28+. -
Statistical Physics Matthew Wingate∗ 19 January 2010 ∗Comment &…
www.damtp.cam.ac.uk/user/wingate/Notes/StatPhys/canonical.pdf19 Jan 2010: 2(2.1.19). = 〈E2〉 〈E〉2 = 〈(E 〈E〉)2〉 = (E)2. (2.1.20). 2 CANONICAL ENSEMBLE 11. -
gmu_blue_gradient
www.damtp.cam.ac.uk/user/astro/conference_web/talks/Dere_Mason2010.pdf22 Nov 2010: Slide 17. Slide 18. Slide 19. Slide 20. Slide 21. -
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: t) =12π. 1(it)3. b′′′(ξ)eiξt dξ. and hence. |t|4|(t)|2 dt <. (20). ... Soviet Physics JETP 40 (1963), 709–719. [20] H. Widom, On a class of integral operators with discontinuous symbol. -
Solar Flare Par*cle Accelera*on ‐ a spectroscopic viewpoint …
www.damtp.cam.ac.uk/user/astro/conference_web/talks/Fletcher_Mason2010.pdf22 Nov 2010: The term ‘flare lines’ usually refers to the highly-ionised states present at 10-20 MK (corona). ... Krucker et al (2009) Jan 20 ‘05 flare. SXR flare spectroscopy. -
Adcock_Hansen_JFAA.dvi
www.damtp.cam.ac.uk/user/na/NA_papers/NA2010_07.pdf10 Dec 2010: 0AMS classification:94A20, 65T99, 47A99, 42C40, 42A10. 1. The well known NS-Sampling Theorem [18, 20, 23, 24, 28] states that if. ... f f̃‖L(R) 2T. B(1 Kn,m)‖Pn β‖l2(N),. (4.20). whereKn,m is as in (4.6). -
Preparing for our futures: what do YOU think? An ...
www.damtp.cam.ac.uk/user/pvl/PLANNING_OUR_FUTURES/21.9.10_poster.pdf11 Sep 2010: 20.00 Breakout groups21.00 Report back: Breakout Group Reporters21.25 Summary: Peter Landshoff (CambridgePPF)21.30 Ends. -
Cambridge_14sep10
www.damtp.cam.ac.uk/user/astro/conference_web/talks/Banerjee_Mason2010.pdf22 Nov 2010: Cadence. Exp. time. Spatial resolutio. n. TRACE Images 13:00:17.000 - 20:59:32.000. ... Summary We found propagating intensity disturbances from the TRACE. images with projected speed ranges from 20-80 km/s and periodicities from 5-9 min. -
Statistical Physics Matthew Wingate∗ 2 February 2010 ∗Comment &…
www.damtp.cam.ac.uk/user/wingate/Notes/StatPhys/thermo2.pdf2 Feb 2010: 5.1.20). Set x = f and y = g to obtain. -
EUV spectral lines properties in impulsively heated multi-stranded…
www.damtp.cam.ac.uk/user/astro/conference_web/talks/Susino_Mason2010.pdf22 Nov 2010: Peter 2010). – Persistent red-shifts (10-20 km/s) in lines at TR temperatures (e.g. -
From high oscillation to rapid approximation II:Expansions in…
www.damtp.cam.ac.uk/user/na/NA_papers/NA2010_02.pdf16 Mar 2010: 13. 20 40 60 80 100. 0.05. 0.10. 0.15. 0.20. 20 40 60 80 100. ... 20 40 60 80 100. 0.05. 0.10. 0.15. 20 40 60 80 100. -
Invpend.dvi
www.damtp.cam.ac.uk/user/na/NA_papers/NA2010_05.pdf4 May 2010: ps1,m = i. m. [. p′s,m bs,m[h]. r=. ar(t)bs,mr[f]. ]. (20). ... Royal Soc. A, 461:1383—1399, 2005. [20] D. R. Merkin.Introduction to the Theory of Stability. -
Non-thermal hydrogen excitation and ionization in the flare 25 July…
www.damtp.cam.ac.uk/user/astro/conference_web/talks/Zharkova_Mason2010.pdf22 Nov 2010: 20. H line intensity (non-thermal thermal excitation). Kernels 1 и 3 (fit very well electrons are the agents). -
Klimchuk_Mason2010
www.damtp.cam.ac.uk/user/astro/conference_web/talks/Klimchuk_Mason2010.pdf22 Nov 2010: also Del Zanna (2008). C IV (1548) Doppler Shifts. Klimchuk (1987) Relative Doppler shift 20 km/s. -
On the convergence of expansions in polyharmonic eigenfunctions Ben…
www.damtp.cam.ac.uk/user/na/NA_papers/NA2010_06.pdf22 Jun 2010: 4. 20 40 60 80 100. 0.5. 1.0. 1.5. 2.0. 2.5. ... Let us first recall some theory of Birkhoff expansions (see [20], for example). -
DOI: 10.1126/science.1190653 , 356 (2010); 330Science et al.Andrew A. …
www.damtp.cam.ac.uk/user/mem/co2-main-ct-knob-lacis-sci10.pdf5 Dec 2010: 20. S. A. E. Marras, F. R. Kramer, S. Tyagi, Nucleic Acids Res.30, e122 (2002). ... typical for theinterglacial maximum, and still the atmosphericCO2 control knob is now being turned faster thanat any time in the geological record (20). -
J Eng Math (2010) 68:279–289DOI 10.1007/s10665-010-9379-7 Determining …
www.damtp.cam.ac.uk/user/hinch/publications/JEngMath68_279.pdf8 Nov 2010: p = p0((. ρ. ρ0. )γ 1. ), (20). where p0 , ρ0 and γ are all constants. ... 123. 288 E. J. Hinch. Table 1 Murnaghan fit (20)for Pb753 with ρ0 = 11.34 Range of ρ p0 γ Rms residual. -
Spectral theory of large Wiener–Hopf operators with complex-symmetric …
www.damtp.cam.ac.uk/user/na/NA_papers/NA2010_09.pdf12 Nov 2010: 10. Figure 3.2: The eigenvalues, denoted by small discs and overlaid on R(a), for τ = 20, 50, 100. ... w(n) zk,τ| (K. τ. )n|z(0) zk,τ| = O. (1. τn1. ). (5.4). 20. We claim thatz(n) = w(n) O(e2δτ ). (5.5). By Lemma 4.3,. -
` Prominence plasma diagnostic with EIS/HinodeN. Labrosse(1), B.…
www.damtp.cam.ac.uk/user/astro/conference_web/talks/Labrosse-poster-2.pdf22 Nov 2010: We obtained values of 20-40 km s-1, but no discernible trend was found. -
Stable reconstructions in Hilbert spaces and the resolution of ...
www.damtp.cam.ac.uk/user/na/NA_papers/NA2010_10.pdf30 Nov 2010: 600. 800. 10 20 30 40 50. 0.1. 0.2. 0.3. 0.4. ... 15. 20 40 60 80. 0.5. 1.0. 1.5. 20 40 60 80. -
Phillips_Mason2010
www.damtp.cam.ac.uk/user/astro/conference_web/talks/Phillips_Mason2010.pdf22 Nov 2010: Active region spectrum 160-180 Å: CHIANTI simulation 4. For temperatures in the 5-20 MK range, Fe is ionized to much higher stages: Fe XVIII – Fe XXV. -
Parenti_Mason2010
www.damtp.cam.ac.uk/user/astro/conference_web/talks/Parenti_Mason2010.pdf22 Nov 2010: 00). Diffuse background emission only 20-30 % less intense than the structured AR. -
531.tif
www.damtp.cam.ac.uk/user/gold/pdfs/teaching/ufk_papers/nanopores/hall.pdf13 Nov 2010: on Septem. ber 20, 2010jgp.rupress.org. Dow. nloaded from. Published October 1, 1975. ... New York. on Septem. ber 20, 2010jgp.rupress.org. Dow. nloaded from. Published October 1, 1975. -
%% PPLANE file %% H.name = 'ML.pps'; H.xvar = ...
www.damtp.cam.ac.uk/user/sje30/teaching/r/Rfiles/ML.pps6 Oct 2010: PPLANE file %% H.name = 'ML.pps'; H.xvar = 'v'; H.yvar = 'w'; H.xder = '(1/20) (90-gca0.5(1tanh((v1.2)/18))(v-120)-8w(v84)-2(v60))'; H.yder = ' ... phi(0.5(1tanh((v-2)/30))-w)cosh((v-2)/60)'; H.pname = {'gca','','phi','','',''}; H.pval = {'4.4','','0.04', -
Culhane_Final
www.damtp.cam.ac.uk/user/astro/conference_web/talks/Culhane_Mason2010.pdf22 Nov 2010: S1. Flares and Magnetic Reconnection – EIS EUV Spectra. Outflow. • B9.5 long duration flare on19-MAY-2007 (Hara et al.): Impulsive phase peak 12:51:20 UT - STEREO, RHESSI, TRACE and ... 20. Conclusions • Although discovered through visible -
Four–dimensional metrics conformal to Kähler
www.damtp.cam.ac.uk/user/md327/Dun_Tod_Math_Proc_final.pdf8 Apr 2010: Quant. Grav. 20 (2003), 4995–5016.[16] G. PAPADOPOULOS. Elliptic monopoles and (4, 0)-supersymmetric sigma models with torsion. ... Trans. Amer. Math. Soc. 331 (1992), 653–661.[20] M. PRZANOWSKI. Killing vector fields in self-dual, Euclidean Einstein -
Excitation of the Fe XIV spectrum in the Sun, ...
www.damtp.cam.ac.uk/user/astro/conference_web/talks/Storey_Mason2010.pdf22 Nov 2010: Excitation of the Fe XIV spectrum in the Sun, stars and Seyfertgalaxies: reconciling theory, observations and experiment. Peter Storey, UCL. 1. Introduction. • Observational background• Modelling Seyfert spectra• Theoretical work on the Fe XIV -
Mitra-Kraev_Mason2010
www.damtp.cam.ac.uk/user/astro/conference_web/talks/Mitra-Kraev_Mason2010.pdf22 Nov 2010: 4. Cooler plasma (0.8—2 MK, Fe VII--Fe XIV) unaffected. Ne from Fe XIV 264.79/274.20. -
Estimating the Persistence Length of a Worm-Like Chain Molecule ...
www.damtp.cam.ac.uk/user/gold/pdfs/teaching/ufk_papers/DNA/bouchiat.pdf15 Nov 2010: Macromolecules.27. 5623–5625. The interpolation formula pro-posed is: log10(2FLp kBT) 5 20.1097t. ... 3 1 0.4509t2 1 1.373t 1 0.02 20.038/(t 1 0.018) witht 5 2log10(1 2 z&/L0). -
Cross-color
www.damtp.cam.ac.uk/user/astro/conference_web/talks/Andretta_Mason2010.pdf22 Nov 2010: Slide 19. Slide 20. Slide 21. Slide 22. Slide 23. Slide 24. -
Cambridge_2010_elena
www.damtp.cam.ac.uk/user/astro/conference_web/talks/Dzifcakova_Mason2010.pdf22 Nov 2010: The 20 level model of Si III is included in CHIANTI. -
Proc. Natl. Acad. Sci. USAVol. 94, pp. 6185– 6190, ...
www.damtp.cam.ac.uk/user/gold/pdfs/teaching/ufk_papers/DNA/baumann.pdf18 Nov 2010: Twenty-five micromolar spermi-dine and 5 mM Co(NH3)631 are the critical concentrationsrequired to condense DNA under these buffer conditions (20,21). ... dichroism and viscometry studies of T7 DNA showedthat a precondensation spermidine concentration of -
Spatial pattern formation and polarization dynamics of a…
www.damtp.cam.ac.uk/user/ngb23/publications/spinor-josephson.pdf27 Jun 2010: Assuming no other symmetry-breaking terms, the linearlypolarized condensate can have independent vortices of theleft- and right-circularly polarized components;19 suchpolarization-dependent phase winding has recently beenobserved.20 These -
Origin of the electrophoretic force on DNA in solid-state nanopores
www.damtp.cam.ac.uk/user/gold/pdfs/teaching/ufk_papers/nanopores/vandorp.pdf2 Nov 2010: V. 1 )F m. ech. (pN. ). R (nm). 30 40 500 10 20. ... Gen. Physiol. 66,531–532 (1975). 20. Netz, R. Polyelectrolytes in electric fields. -
Reproducible Imaging and Dissection of Plasmid DNA Under Liquid with…
www.damtp.cam.ac.uk/user/gold/pdfs/teaching/ufk_papers/AFM/hansma.pdf23 Sep 2010: Plasmid strands are 3 to 6 nm wide in (A) to (D), and 15 to 20 nm in (F). ... DNA is more easily dissect- ed in a 80:20 propanol-water mixture than in propanol alone. -
Biophysical Journal Volume 72 March 1997 1335-1346 Stretching DNA ...
www.damtp.cam.ac.uk/user/gold/pdfs/teaching/ufk_papers/DNA/wang.pdf13 Nov 2010: Clamp Off Clamp On. 0 20 40 60 80 100 120 0 20 40 60 80 100 120. ... 50. 40. 30. --. z. aL)L.0U. 20. 10. 0. Force-extension relations. -
Mesoscale conformational changes in theDNA-repair complex…
www.damtp.cam.ac.uk/user/gold/pdfs/teaching/ufk_papers/AFM/moreno.pdf22 Oct 2010: a, Definition of angle a ( (a1 þ a2)/2) and distance d.Movies composed of 6–20 frames were acquired for 17 different hR/Mmolecules. ... A 20 ml portion of the dilutedsolution (400 ng of protein complex in 150 mM KCl, 25 mM Tris-HCl pH 8.0,10% glycerol)
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