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1 - 10 of 52 search results for KaKaoTalk:ZA31 24 24 |u:www.damtp.cam.ac.uk where 0 match all words and 52 match some words.

  1. Results that match 2 of 3 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: 30.94268 12.20211 165.4088 14.02198 102.1661 22.39954 130.5360 24.54925 54.39669 27.35860 55.83458 18.97185 260.9365 28.02304 194.9137 ... 5112 155.7039 259.5173 223.7271 266.5150 248.4850 266.6068 122.2994 271.7742 286.1407 280.3929 241.9675 282.2188 162

  3. www.damtp.cam.ac.uk/user/sje30/data/mosaics/w81_scan/w81s1on.txt

    www.damtp.cam.ac.uk/user/sje30/data/mosaics/w81_scan/w81s1on.txt
    5 Feb 2015: 277.1 558.79 317.32 36.05 325.27 668.09 344.24 134.28 340.67 316.73 355.22 397.9 361.75 491.87 386.29

  4. PowerPoint Presentation

    www.damtp.cam.ac.uk/user/astro/cl7/talks/P3_8.pdf
    27 Jul 2015: We examine an extended coronal source6 (2005 Aug 23) with little footpoint emission (left panel) and a more common looptop and footpoint event7 (2011 Feb 24, right panel). ... f). (g) (h). For the 2011 Feb 24 flare we see something close to a power law.

  5. Coronal Loop Workshop VII

    www.damtp.cam.ac.uk/user/astro/cl7/program.html
    16 Aug 2015: G. R. Gupta, D. Tripathi & H. E. Mason. P1.24. CHIANTI version 8.

  6. Nanoflare vs footpoint heating : Observational signatures

    www.damtp.cam.ac.uk/user/astro/cl7/talks/CT1_4.pdf
    23 Jul 2015: 335 - 193 79.7% 31.2% 24.8% 44.0%. 335 - 171 72.1% 23.9% 23.0% 53.1%. ... 335 - 171 62.8% 29.4% 7.8%. 211 - 193 24.7% 40.8% 34.4%.

  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: 11:00 11:30 12:00 12:30 13:00Start Time (29Apr15 10:30:01). 2022. 24. 2628.

  8. 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: 32. 24. 16. 8. 0. 16. Modeling results: high umbral loops. ... 6.0. 6.1. 6.2. 6.3. 6.4. 6.5. (d) Log (T) K. 07 Jul 2014 10:24 UT Another Time Frame.

  9. 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: rMHD 24 Mm. 24 Mm. 17 Mm. R=700 Mm. CZ. corona. • ... chromospheretransition region. corona. Computational setup. 24 Mm. 17 Mm. • domain size: 24x24x17 Mm3. •

  10. 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 21. Slajd 22. Slajd 23. Slajd 24. Slajd 25. Slajd 26.

  11. Geometric pumping in autophoretic channels

    www.damtp.cam.ac.uk/user/lauga/papers/107.pdf
    4 Aug 2015: pattern-ing the particle surface with active and passive sites (e.g. Janusparticles),23,24,28 (ii) spontaneous symmetry-breaking resultingfrom the advection of the field responsible for the phoreticresponse by ... K. Sia and G. M. Whitesides,

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