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1 - 20 of 37 search results for KaKaoTalk:vb20 200 |u:www.damtp.cam.ac.uk where 0 match all words and 37 match some words.

  1. Results that match 1 of 2 words

  2. www.damtp.cam.ac.uk/user/sje30/data/mosaics/hor/w00h72.txt

    www.damtp.cam.ac.uk/user/sje30/data/mosaics/hor/w00h72.txt
    5 Feb 2015: 174.3860 212.0221 183.4615 275.1014 184.2850 184.2154 184.4135 244.6897 187.3142 70.22635 190.3387 94.84615 197.1700 121.0863 200.5851

  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. 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: In particular, strong blueshifts ( 200 km/s) are simultaneously observed in both IRIS Fe XXI 1354 A and HINODE/EIS Fe XXIII 263 A hot (>10 MK) emission lines at one ... Large blue shifts (200 km/s) in IRIS Fe XXI and EIS Fe XXIII high temperature lines

  5. Particle dynamics in a non-flaring solar active region

    www.damtp.cam.ac.uk/user/astro/cl7/talks/P1_4.pdf
    22 Jul 2015: 30. -80. -30. So. lar-. Y [. arc. se. c]. a ). 100 150 200 250. Sola r-X [ar csec]. b). S L1. ... S L2. SL3. CL1. 100 150 200 250. S olar-X [a rcsec].

  6. Department of Mathematics,Center for mathematicalPlasma-Astrophysics…

    www.damtp.cam.ac.uk/user/astro/cl7/talks/P3_2.pdf
    26 Jul 2015: 0. 5. 190 200 210 220 230 240 250 260. Ma. ... 15. 20. 25. 30. 35. 40. 45. 50. 190 200 210 220 230 240 250 260.

  7. SDO/A IA, Hinode/XRT, and NuSTAR For the poster and ...

    www.damtp.cam.ac.uk/user/astro/cl7/talks/P1_21.pdf
    22 Jul 2015: 2014, Sol. Phys., 289, 1029. AIA FeXVIII 29Apr2015 10:30:01.120 UT. 100 200 300 400 500X (arcsecs). ... rcse. cs). AIA FeXVIII 29Apr2015 10:30:01.120 UT. 100 200 300 400 500X (arcsecs).

  8. PowerPoint Presentation

    www.damtp.cam.ac.uk/user/astro/cl7/talks/P3_6.pdf
    26 Jul 2015: The time was broken into 200 s for the linear increase, 100 s for the plateau, and 200 s for the linear decrease.

  9. Efficient Modeling of Two-fluid Coronal Plasma: Effects of Electron…

    www.damtp.cam.ac.uk/user/astro/cl7/talks/P1_26.pdf
    22 Jul 2015: 200 s)I Single-fluid models tacitly assume electron and ion populations in equilibrium violated if heating. ... 1(b) Same as Fig. 1(a), but for aseries of 23 square pulses, each lasting 200 s with amplitudes chosen from a power-law distribution.

  10. Instabilities of a thin coating on a vertical fibre; Newtonian,…

    www.damtp.cam.ac.uk/user/hinch/talks/ICL2015.pdf
    4 Nov 2015: 100. 200. 300. 400. 500. 600. 700. 800. 0 0.5 1 1.5 2. ... 150. 200. 250. 300. 350. -4 -2 0 2 4 6 8 10 12.

  11. 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

  12. Emission measure distribution of nanoflare-heated coronal loops…

    www.damtp.cam.ac.uk/user/astro/cl7/talks/P1_10.pdf
    30 Jul 2015: 2.2 Critical condition:. We model the nanoflares with 200 s triangular heating functions.

  13. Coronal_loops_7_Reva

    www.damtp.cam.ac.uk/user/astro/cl7/talks/P1_18.pdf
    30 Jul 2015: 4) The loops' intensity gradually decreases over approximately 1 hour. All four arcades had similar sizes: the loop length was 170 Mm, and the arcade length was 200 Mm (see Figure

  14. Instabilities of a thin coating on a vertical fibre; Newtonian,…

    www.damtp.cam.ac.uk/user/hinch/talks/Leeds2015.pdf
    10 Oct 2015: 100. 200. 300. 400. 500. 600. 700. 800. 0 0.5 1 1.5 2. ... 150. 200. 250. 300. 350. -4 -2 0 2 4 6 8 10 12.

  15. 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: ty w. ith N. orm. al F. it. 0.000.050.100.150.200.25. 60 65 70 75 80. ... Alto 1. Soprano 2. 60 65 70 75 80. 0.000.050.100.150.200.25. Soprano 1.

  16. Heating Mechanisms (Reconnection and Waves) 1 M. Asgari-Targhi…

    www.damtp.cam.ac.uk/user/astro/cl7/talks/IT1_1.pdf
    21 Jul 2015:  At present the spatial resolution of some of the DC models (Binger and Peter 2011) is 200 km.

  17. Description of MEA data for Charlesworth et al (2015) ...

    www.damtp.cam.ac.uk/user/sje30/papers/charlesworth2015_data.pdf
    17 Sep 2015: Electrodes were aligned in asquare array, spaced 200 um apart.). 1.

  18. Do Dissolving Objects Converge to a Universal Shape?Elias Nakouzi,†…

    www.damtp.cam.ac.uk/user/gold/pdfs/dissolution.pdf
    1 May 2015: b) Poly(ethyleneglycol) cylinder at 5, 150, 200, and 250 min. Individual image size: 14cm 4 cm.

  19. on June 3, 2015http://rsif.royalsocietypublishing.org/Downloaded from …

    www.damtp.cam.ac.uk/user/gold/pdfs/metachronal_jrsi.pdf
    3 Jun 2015: 200. 0. 200. 100. 0. colonyaxis. uÒtur. uq. t = 0 ms 6 ms 12 ms 18 ms 24 ms. ... beats0 200 400 600. no. beats. no. beats0 10 20 30 40 50 0 20 40 60 80 100.

  20. Instability of a Möbius Strip Minimal Surface and a ...

    www.damtp.cam.ac.uk/user/gold/pdfs/meeks_mobius.pdf
    24 Mar 2015: Comput. Phys. 200, 299 (2004). [12] D. Leppinen and J. R.

  21. on May 16, 2015http://rsfs.royalsocietypublishing.org/Downloaded from …

    www.damtp.cam.ac.uk/user/gold/pdfs/streaming_focus.pdf
    16 May 2015: eH. uH. uyej. 400. 0.5. 0.006 200. –200. –400. 0. 60. ... x (µm)–400 –200 200 4000. –1. 1. –10 –5 0. z (mm).

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