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4 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.

6 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

4 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.

11 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.

18 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.

12 Jan 2010: 4.75 4.0 102 7.3 1010. Table: Errors for n = 20.

23 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

6 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',

18 Feb 2010: n = 10 104 sec., n = 20 17 min, n = 30 4 105 years.

22 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,.

23 Sep 2010: The ODE (20) has an elementary solution given by certain rational curves which will be analysedin the next section. ... which is the ODE (20) from Theorem 5.2. Page 14 of 32 M.

22 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”.

27 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.

22 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+.

22 Nov 2010: Slide 17. Slide 18. Slide 19. Slide 20. Slide 21.

5 Nov 2010: Received 20 July 2010; accepted 22 July 2010). Batchelor made his name with research in turbulence in the 1940s and 1950s. ... Fluid Mech. 20, 111–157. Davis, R. H. & Acrivos, A. 1985 Sedimentation of non-colloidal particles at low Reynolds numbers.Annu

17 Nov 2010: 20. 40. 60. 80. 100. 120. 140. 0 20 40 60 80 1000. ... 20. 40. 60. 80. 100. 120. 140. Interparticle distance (aφ–1/3). Inte.

22 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.

30 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.

11 Sep 2010: 20.00 Breakout groups21.00 Report back: Breakout Group Reporters21.25 Summary: Peter Landshoff (CambridgePPF)21.30 Ends.

10 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).

22 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.

22 Nov 2010: Peter 2010). – Persistent red-shifts (10-20 km/s) in lines at TR temperatures (e.g.

22 Nov 2010: 20. H line intensity (non-thermal thermal excitation). Kernels 1 и 3 (fit very well  electrons are the agents).

16 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.

4 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.

22 Nov 2010: also Del Zanna (2008). C IV (1548) Doppler Shifts. Klimchuk (1987) Relative Doppler shift 20 km/s.

22 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).

5 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).

22 Nov 2010: We obtained values of 20-40 km s-1, but no discernible trend was found.

12 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,.

30 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.

22 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.

22 Nov 2010: 00).  Diffuse background emission only 20-30 % less intense than the structured AR.

13 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.

10 Sep 2010: 17:00 - 17:20. Conference Reception 17:45 - 19:00. Tuesday - 14th September - 2010. ... Stephen Bradshaw Non-equilibrium process in the Solar Corona 16:20 - 16:40.

22 Nov 2010: 4. Cooler plasma (0.8—2 MK, Fe VII--Fe XIV) unaffected. Ne from Fe XIV 264.79/274.20.

22 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

22 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

8 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

8 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.

15 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).

22 Nov 2010: Slide 19. Slide 20. Slide 21. Slide 22. Slide 23. Slide 24.

22 Nov 2010: The 20 level model of Si III is included in CHIANTI.

18 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

27 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

2 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.

23 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.

13 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.

22 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)