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1 - 10 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

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