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New Insights into the Sun’s Photosphere Dynamics Offered by New Solar Telescope of BBSO

New Insights into the Sun’s Photosphere Dynamics Offered by New Solar Telescope of BBSO. Valentina Abramenko, Vasyl Yurchyshyn, Philip R. Goode and the NST team Big Bear Solar Observatory, CA avi@bbso.njit.edu. Big Bear Solar Observatory. 7/02/2011.

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New Insights into the Sun’s Photosphere Dynamics Offered by New Solar Telescope of BBSO

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  1. New Insights into the Sun’s Photosphere Dynamics Offered by New Solar Telescope of BBSO Valentina Abramenko, Vasyl Yurchyshyn, Philip R. Goode and the NST team Big Bear Solar Observatory, CA avi@bbso.njit.edu Big Bear Solar Observatory 7/02/2011 XXV IUGG/IAGA, Melbourne, Australia

  2. New Solar Telescope at Big Bear 7/02/2011 XXV IUGG/IAGA, Melbourne, Australia

  3. 7/02/2011 XXV IUGG/IAGA, Melbourne, Australia

  4. Coude room optical layout 7/02/2011 XXV IUGG/IAGA, Melbourne, Australia

  5. Magnetic Fields Measurements from NST and SDO NST InfraRed Magnetogram SDO magnetigram 7/02/2011 XXV IUGG/IAGA, Melbourne, Australia

  6. Hinode Satellite (Left) and NST (Right) Images of the Sun the Same Time/Place (Abramenko et al. 2010, ApJL, 725) Hinode/G-band NST TiO 7/02/2011 XXV IUGG/IAGA, Melbourne, Australia

  7. Bright points (magnetic flux tubes) are NOT ribbons, but always form chains of beads

  8. NST observations verify simulations of granula evolution : formation of bright granula lane moving inside the granula is accompanied by emergence of horizontal rotating vortex tube and tiny jets (Yurchyshyn et al. 2011 ApJL, accepted) 7/02/2011 XXV IUGG/IAGA, Melbourne, Australia

  9. Pores and penumbra formation , photospheric signatures of flux emergence (Lim et al, ApJ submitted) 7/02/2011 XXV IUGG/IAGA, Melbourne, Australia

  10. Dynamics and statistics of photospheric bright points (BPs) A set of 648 TiO images: AO corrected Speckle reconstructed Aligned Destretched Image size: 14 x 14 Mm, or 510 x 510 pixels Cadence 10 s 17539 BPs were detected and tracked 7/02/2011 XXV IUGG/IAGA, Melbourne, Australia

  11. 77 km Size distribution of BPs: minimum size of flux tubes is not reached yet (Abramenko et al. 2010, ApJL, 725) 7/02/2011 XXV IUGG/IAGA, Melbourne, Australia

  12. Magnetic diffusion in the photosphere occur in a super-diffusion regime on scales below 600 km and shorter than 10 min (Abramenko et al. under preparation) Details: Tuesday, Jul 5, 16:30 talk in this room 7/02/2011 XXV IUGG/IAGA, Melbourne, Australia

  13. 7/02/2011 XXV IUGG/IAGA, Melbourne, Australia

  14. Diffusivity: some definitions: 7/02/2011 XXV IUGG/IAGA, Melbourne, Australia

  15. Details: Tuesday, Jul 5, 16:30 talk in this room 7/02/2011 XXV IUGG/IAGA, Melbourne, Australia

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