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1 - 10 of 72 search results for TALK:PC53 20 |u:www.damtp.cam.ac.uk where 0 match all words and 72 match some words.

  1. Results that match 1 of 2 words

  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.

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