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  2. www.damtp.cam.ac.uk/user/sje30/data/mosaics/hor/w00h71.txt

    www.damtp.cam.ac.uk/user/sje30/data/mosaics/hor/w00h71.txt
    5 Feb 2015: 34649 76.75254 19.35413 114.5557 19.55190 209.9197 20.88294 280.8345 22.38324 17.63480 23.10568 221.0292 23.55057 159.4284 25.3211 290.0137 ... 25.75550 182.9498 28.98305 234.4741 30.25903 146.4806 32.29067 89.69438 34.69780 67.14715 36.27759 246.7832
  3. Dynamic evolution of EUV loops Yin Zhang, Baolin Tan ...

    www.damtp.cam.ac.uk/user/astro/cl7/talks/P1_6.pdf
    26 Jul 2015: 0 50 100 150 200 250-20. -10. 0. 10. 20. 30. ... 0 50 100 150 200 250-40. -20. 0. 20. 40. 60.
  4. Coronal Loop Workshop VII

    www.damtp.cam.ac.uk/user/astro/cl7/program.html
    16 Aug 2015: S. Regnier, R. W. Walsh & C. E. Alexander. P1.20.
  5. Non-Thermal Motions in the Hot Cores of Solar Active ...

    www.damtp.cam.ac.uk/user/astro/cl7/talks/CT1_2.pdf
    21 Jul 2015: Chromospheric evaporation in response to coronal nanoflares: 20-36km/s @ 1.1-5.6MK @ loop tops (Patsourakos & Klimchuk 2006) [Increasing trend with temperature]. ... Skylab: 10-20 km/s in coronal UV lines (Cheng et al.
  6. Magnetic Coupling between Chromosphere and Corona Measured with HMI,…

    www.damtp.cam.ac.uk/user/astro/cl7/talks/P2_1.pdf
    27 Jul 2015: 0. 10. 20. 30. 40. 50. 60. 70. E fre. e [10. ... 29]. 0. 10. 20. 30. 40. 50. 60. 70. E fre. e [10.
  7. AbstractTo simulate the energy balance of coronal plasmas on ...

    www.damtp.cam.ac.uk/user/astro/cl7/talks/P1_25.pdf
    26 Jul 2015: 20. 30. 40. 50. 60. Tim. e [H. r]. 0 20 40 60 80 100 120 140S [Mm]. ... B0/L. 1 10 100 1000B0/L [Mas]. 0.0. 0.1. 0.2. 0.3. λQ [. RS]. WTD HeatingEmpirical Heating. Tmax [MK]. 0 20 40 60 80 100Loop Index.
  8. December 7, 1999, 6.1 New Start Proposal for FY01 MODELING MAGNETIC…

    www.damtp.cam.ac.uk/user/astro/cl7/talks/CT3_3.pdf
    23 Jul 2015: Steady-State Ohmic Heating. At 10 times higher resistivity:. Maximum tilt decreases from 20 to 3.
  9. Coronal_loops_7_Reva

    www.damtp.cam.ac.uk/user/astro/cl7/talks/P1_18.pdf
    30 Jul 2015: 3) The loops' intensity increased and reached maximum after 5-20 minutes. ... On the EIT 195 Å images, the precursor looked like a loop with the size 20 Mm, but the arcade was invisible (see Figure 2 right).
  10. On the modeling of active region EUV and X-Ray emission Jaroslav…

    www.damtp.cam.ac.uk/user/astro/cl7/talks/P1_16.pdf
    30 Jul 2015: More details at: Dudík et al. 2014 (Astrophys. J., 796, 20)).
  11. Particle dynamics in a non-flaring solar active region

    www.damtp.cam.ac.uk/user/astro/cl7/talks/P1_4.pdf
    22 Jul 2015: sub.). Ô. 2000 particles evenly distributedthroughout lower corona. Ô. Uniform initial pitch angle (45)and kinetic energy (20 eV),simulated for 10 s. ... 2011 ApJ, 729, 101[19] Gordovskyy et al., 2014 A&A, 561, A72[20] Grady, K.
  12. Slide 1

    www.damtp.cam.ac.uk/user/astro/cl7/talks/P1_19.pdf
    28 Jul 2015:  Red-shifts and blue-shifts (up to 20 kms-1) can be reproduced for the different simulated Hinode/EIS.
  13. Instabilities of a thin coating on a vertical fibre; Newtonian,…

    www.damtp.cam.ac.uk/user/hinch/talks/Leeds2015.pdf
    10 Oct 2015: Fluid Mech. 1994. 0. 20. 40. 60. 80. 100. 0 0.5 1 1.5 2. ... 1. 2. 3. 4. 5. 6. 7. 8. 10 20 30 40 50 60.
  14. Hi-C observations of an active region corona, and investigation of…

    www.damtp.cam.ac.uk/user/astro/cl7/talks/CT1_6.pdf
    22 Jul 2015: Suppression of Heating of Coronal Loops Rooted in Opposite Polarity Sunspot Umbrae. Sanjiv K. Tiwari,. (J. K. Thalmann, A. R. Winebarger, N. K. Panesar#, R. L. Moore#). Marshall Space Flight Center. 21 Jul 2015 Loops VII, Univ. of Cambridge. sanjiv.k
  15. 31 Dec 2015: The vibration of the bubble interface underultrasonic forcing results in a strong “acoustic-streaming”jet [20]. ... dary acoustic) streaming, is then dominant [20]. It occursin viscous boundary layers near walls (see Ref.
  16. Slide 1

    www.damtp.cam.ac.uk/user/astro/cl7/talks/P1_5.pdf
    28 Jul 2015: Fig. 5), we determine that the temperature of the. plasma is between 15 MK and 20 MK.
  17. Instabilities of a thin coating on a vertical fibre; Newtonian,…

    www.damtp.cam.ac.uk/user/hinch/talks/ICL2015.pdf
    4 Nov 2015: Fluid Mech. 1994. 0. 20. 40. 60. 80. 100. 0 0.5 1 1.5 2. ... 1. 2. 3. 4. 5. 6. 7. 8. 10 20 30 40 50 60.
  18. A Computational Method for Modelling Chromospheric Evaporation

    www.damtp.cam.ac.uk/user/astro/cl7/talks/P2_6.pdf
    23 Jul 2015: Wavefront location xf (t ) (solid line) and STS approximation(asterisks) with resolution : a) Nx = 20, Nt = 50, b) Nx =40, Nt = 100, c) Nx = 80, Nt = 200, d) Nx = 160, Nt
  19. A reciprocal theorem for boundary-driven channel flows

    www.damtp.cam.ac.uk/user/lauga/papers/111.pdf
    31 Dec 2015: This approachmakes an extensive use of the reciprocal theorem for Stokes flows.20. ... Kim and S. J. Karrila, Microhydrodynamics (Dover Publications, Inc., New York, 2005).20 L.
  20. Nanoflare vs footpoint heating : Observational signatures

    www.damtp.cam.ac.uk/user/astro/cl7/talks/CT1_4.pdf
    23 Jul 2015: measured and POSITIVE. 335 - 211 55.2% 54.0% 16.3% 29.6%. 335 - 193 61.9% 45.7% 20.4% 33.8%.
  21. Standard Model Mathematical Tripos, Part IIIDr M B Wingate ...

    www.damtp.cam.ac.uk/user/wingate/Notes/StdM/sheet2.pdf
    8 Feb 2015: 30) b Tr(Φ. 20). (µ may be regarded as a Lagrange multiplier for the condition Tr(Φ) = 0 whenvarying V (Φ)).
  22. Heating Mechanisms (Reconnection and Waves) 1 M. Asgari-Targhi…

    www.damtp.cam.ac.uk/user/astro/cl7/talks/IT1_1.pdf
    21 Jul 2015: The X-ray emission from loops is highly variable:. 3. SDO observation of an active region NOAA 11564 on 2012 September 7 at 7:20 UT. ... Waves Heating Models. Alfven Wave Turbulence Model. 20. Simulations of Alfven waves in coronal loops (van
  23. Set of observationsSet of observations ● IRIS: 14:04- 17:44 ...

    www.damtp.cam.ac.uk/user/astro/cl7/talks/P1_29.pdf
    28 Jul 2015: EIS: 11:02-17:27 UT 20-steps raster, cadence 212 s, exposure time 9s.
  24. Miniature coronal loops Krzysztof Barczyński1 Hardi Peter1 1) Max ...

    www.damtp.cam.ac.uk/user/astro/cl7/talks/CT2_3.pdf
    22 Jul 2015: Slajd 15. Slajd 16. Slajd 17. Slajd 18. Slajd 19. Slajd 20.
  25. Classical transition region vs. low-lying loops Jul 22, 2015 ...

    www.damtp.cam.ac.uk/user/astro/cl7/talks/IT2_2.pdf
    22 Jul 2015: 2011b). Wednesday 22 July 15. blue. 0 10 20 30time [min].
  26. Geometric pumping in autophoretic channels

    www.damtp.cam.ac.uk/user/lauga/papers/107.pdf
    4 Aug 2015: f C. ambr. idge. on. 04/0. 8/20. 15 1. 5:21. :05. ... Uni. vers. ity o. f C. ambr. idge. on. 04/0. 8/20.
  27. 4 Aug 2015: However, recenttheoretical investigation suggests that interactions could. have a longer spacial extent and a slower decay rate thanpreviously thought [20]. ... Meanwhile,at large separations the values compare very well, with thelargest discrepancy
  28. Cover Realistic Magnetic Reconnection Processes

    www.damtp.cam.ac.uk/user/astro/cl7/talks/IT3_2.pdf
    23 Jul 2015: N. Shore,22 A. Sillanpää,20 J. Sitarek,1 I. Snidaric,5 D. Sobczynska,9. F. ... L. Takalo,20 H. Takami,19 F. Tavecchio,3 P. Temnikov,21 T. Terzić,5 D.
  29. Instability of a Möbius Strip Minimal Surface and a ...

    www.damtp.cam.ac.uk/user/gold/pdfs/meeks_mobius.pdf
    24 Mar 2015: DOI: 10.1103/PhysRevLett.114.127801 PACS numbers: 68.15.e, 02.40.-k, 47.20.Ky, 83.10.-y. The subject of this Letter lies at the intersection ofseveral branches ... 137 (American Mathemati-cal Society, Providence, RI, 2007). [20] For a summary of open
  30. Are Black Holes Like Metals? David Tong Seoul Na;onal ...

    www.damtp.cam.ac.uk/user/tong/talks/snu.pdf
    28 May 2015: Op;cal Conduc;vity. 0 5 10 15 20 250. 2. 4. 6. ... 20. Hartnoll, 2014. which of these processes describes actual materials? Lesson 2: Incoherent Transport.
  31. Department of Mathematics,Center for mathematicalPlasma-Astrophysics…

    www.damtp.cam.ac.uk/user/astro/cl7/talks/P3_2.pdf
    26 Jul 2015: 15. 20. 25. 30. 35. 40. 45. 50. 190 200 210 220 230 240 250 260. ... 5. 10. 15. 20. 25. 30. 0 900 1800 2700 3600 4500.
  32. PHYSICAL REVIEW E 92, 022701 (2015) Feeding ducks, bacterial ...

    www.damtp.cam.ac.uk/user/gold/pdfs/ducks.pdf
    5 Aug 2015: coli, with v 20 μm/s and τ 1 s, run 20 μm, but it can be considerably longer for otherbacteria [28]. ... 30, 235 (1971). [20] J. D. Murray, Mathematical Biology II Spatial Models andBiomedical Applications, 3rd ed.
  33. Geometric capture and escape of a microswimmer colliding with an…

    www.damtp.cam.ac.uk/user/lauga/papers/105.pdf
    22 Apr 2015: Fig. 6 shows thetrajectories of non-interacting pullers with a 0.8 swimmingtowards a sphere of size A 20. ... Fig. 8provides a general picture of the scattering dynamics, where wex the colloid size to A 20.
  34. 7 Green’s Functions for Ordinary Differential Equations One of ...

    www.damtp.cam.ac.uk/user/dbs26/1BMethods/GreensODE.pdf
    9 Nov 2015: We already have the Green’s function. solution to the homogeneous problem in (7.20), so we simply need to find a solution to. ... sin x. sin 1. 1. xf(ξ) sin(1 ξ) dξ (7.35). using the result (7.20). –
  35. Do Dissolving Objects Converge to a Universal Shape?Elias Nakouzi,†…

    www.damtp.cam.ac.uk/user/gold/pdfs/dissolution.pdf
    1 May 2015: Notice that higher temperatures induce unwantedcaramelization.20 The molten sugar is poured into a cylindrical Teflonmold (length 14 cm and inner diameter 2 cm) until it fills the entirebore volume (approximately ... Phys. Rev. E 2013, 87, 011003.(20)
  36. Stable nonuniform sampling with weighted Fourierframes and recovery…

    www.damtp.cam.ac.uk/research/afha/anders/SAMPTA_Milana.pdf
    30 May 2015: Forpolynomial reconstructions see [19] and [20]. IV. NUGS IN ONE DIMENSIONIn one dimension we take ZK R̂ to be the interval. ... Com-put. Phys., vol. 229, no. 3, pp. 933–946, 2010. [20] B.
  37. Plethora of transitions during breakup ofliquid filamentsJosé Rafael…

    www.damtp.cam.ac.uk/user/hinch/publications/PNAS-2015.pdf
    31 Mar 2015: These satellites aretypically much smaller than the primary drop (20) and almostalways undesirable in applications (2). ... Nat Phys 5:697–702. 20. Collins RT, Harris MT, Basaran OA (2007) Breakup of electrified jets.
  38. Stable nonuniform sampling with weighted Fourierframes and recovery…

    www.damtp.cam.ac.uk/research/afha/people/anders/SAMPTA_Milana.pdf
    30 May 2015: Forpolynomial reconstructions see [19] and [20]. IV. NUGS IN ONE DIMENSIONIn one dimension we take ZK R̂ to be the interval. ... Com-put. Phys., vol. 229, no. 3, pp. 933–946, 2010. [20] B.
  39. Experimental mosaics studied in the Hore, Troy and Eglen ...

    www.damtp.cam.ac.uk/user/sje30/data/mosaics/hore2012_mosaics.pdf
    5 Feb 2015: Define some common functions for plotting.soma.rad <- 20/2 #20 um soma diameter.on.col <- "red"of.col <- "blue"show.on <- function(pts, main) {. symbols(pts, circles = rep(soma.rad,
  40. Banded, stable, skew-symmetricdifferentiation matrices of high order…

    www.damtp.cam.ac.uk/user/na/NA_papers/NA2015_03.pdf
    9 Nov 2015: There are two real zeros.One is close to 0.2144 and the other is (up to 20 digits). ... V̇ CD̂V = F(t), U(0) = U0, (31) advectionnumv. 21. 25 20 15 10 5.
  41. J. Fluid Mech. (2014), vol. 757, pp. 330–353. c© ...

    www.damtp.cam.ac.uk/user/jneufeld/pubfiles/Pegler-2014-1.pdf
    21 Jan 2015: The dimensionless form of the inequality (2.20) is. B < QF < Qmax BD1(1B). ... 1 20. 0.5. 1.0. 0 1 2 0 1 2 3.
  42. on June 3, 2015http://rsif.royalsocietypublishing.org/Downloaded from …

    www.damtp.cam.ac.uk/user/gold/pdfs/metachronal_jrsi.pdf
    3 Jun 2015: roto. rro. tor. 0 5 10 10 20 30 0 1 2 315 20 25 30. ... 0.9. 0.85 10 15. 0.98 1.021. 20 25 30. 102030. 51525.
  43. Green Algae as Model Organisms for Biological Fluid Dynamics

    www.damtp.cam.ac.uk/user/gold/pdfs/green_algae.pdf
    25 Sep 2015: l use. onl. y. FL47CH15-Goldstein ARI 1 December 2014 20:34. 1. ... FL47CH15-Goldstein ARI 1 December 2014 20:34. g h. a b c.
  44. Scientific Programming with R Stephen EglenLaurent Gatto September 6, …

    www.damtp.cam.ac.uk/user/sje30/teaching/r/2015/spr-4up.pdf
    1 Oct 2015: x. [1] 20.00000 24.14214 27.32051 30.00000 32.36068. 62 / 191. ... y. 0 5 10 15 20 25 30. 0.0. 0.5. 1.0.
  45. Continuous Compressed Sensing of Inelastic and Quasielastic Helium…

    www.damtp.cam.ac.uk/research/afha/anders/CS4HAS_Arxiv_2.pdf
    4 Oct 2015: gj =. Nk=N. Aj,kfk, j = 0,. , 2N, gj = ρ̃N (λj,N ), (20). ... 20 40 60 80 1000. 0.2. 0.4. 0.6. 0.8. 1. Frequencies.
  46. Continuous Compressed Sensing of Inelastic and Quasielastic Helium…

    www.damtp.cam.ac.uk/research/afha/people/anders/CS4HAS_Arxiv_2.pdf
    4 Oct 2015: gj =. Nk=N. Aj,kfk, j = 0,. , 2N, gj = ρ̃N (λj,N ), (20). ... 20 40 60 80 1000. 0.2. 0.4. 0.6. 0.8. 1. Frequencies.
  47. Cop yrig ht © 201 3 U nive rsity ...

    www.damtp.cam.ac.uk/user/tong/em/macfarlane.pdf
    13 Jan 2015: 20). Here (17) has been used. Eq. (20) expresses the conservation of charge. ... drop. tterms, and replace (.) by n(.)|. Thus, from (20), we expect that n J|. =
  48. On the modeling of active region EUV and X-Ray emission Jaroslav…

    www.damtp.cam.ac.uk/user/astro/cl7/talks/P3_11.pdf
    26 Jul 2015:  The loop is highly non-Maxwellian, with κ < 2.  Calibration uncertainty is large (20%) and ought to be reduced in future missions.
  49. On fundamentals of models and sampling in compressed sensing ...

    www.damtp.cam.ac.uk/research/afha/people/alexb/papers/CSModels.pdf
    10 Jul 2015: 20. 0. 20. Wx0 thresholded to s = 150. 0 500 1000 1500 2000 2500 3000 3500 4000 45000. ... Magn.Reson. Imaging, 58(6):1182–1195, 2007. [20] C. Poon. On the role of total variation in compressed sensing.
  50. Why geometric numerical integration? A. Iserles & G.R.W. Quispel…

    www.damtp.cam.ac.uk/user/na/NA_papers/NA2015_05.pdf
    17 Dec 2015: x1 = x′1 hx′21 h2x′31 k(x2,x3; h). (2.20). where the function k denotes an integration constant that we can choose appropriately.The simplest VP integrator satisfying ... 20. effective algorithms for the solution of linear systems, computation of
  51. 3 Laplace’s Equation In the previous chapter, we learnt ...

    www.damtp.cam.ac.uk/user/dbs26/1BMethods/Laplace.pdf
    26 Oct 2015: An,m =4. ab. [0,a][0,b]sin. (nπxa. )sin. (mπyb. )f(x, y) dx dy (3.20). ... x2 (λ)(6 λ). 4!x4. (λ)(6 λ)(20 λ)6! x6. Θ1(x) = x (2 λ).

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