a case in point? use of the sst, numerical simulations, and ひので in modelling dynamic fibrils,...
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...a case in point?use of the SST, numerical simulations, and ひ
ので in modelling dynamic fibrils, spicules, and mottles
Romforskningsutvalget ved ITA20-mars 2007
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H-alpha core 4-oct-2005
• Taken at the SST by Luc Rouppe van der Voort and Michiel van Noort
Diffraction limited (0.2”), Ha linecenter at 1 s cadence, from 8:50 to 10:10 UT, m=0.78 (S8, E37)
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Dynamic Fibrils Evolution
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3d MHD simulations
• 3d Oslo Stagger Code; 5th order spatial interpolation, 3d order time stepping
• Non-grey radiative transfer w/ scattering the chromosphere; optically thin radiation in lower transition region and corona
• Thermal conduction along magnetic field
• Transmitting boundaries; allow control of entropy and magnetic field configuration that enters the computational box from below
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Simulated Dynamic FibrilsHansteen, De Pontieu et al. 2006 ApJL 647, L73-L76 De Pontieu, Hansteen et al. 2007 ApJ 655, 624-641
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Observations vs. Simulations xt-plots
• Spicule-like features in simulations - due upwardly propagating shocks -show parabolic paths similar to those observed in DFs, as well as a host of other similarities...
Observations Simulations
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Observations vs. Simulations velocity/deceleration
• The correlation between maximum velocity along a DF and the deceleration is well reproduced by simulations. It is a consequence of the shock acceleration of dynamic fibrils.
Rouppe van der Voort et al. 2007 ApJL, in press
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• Japan/US/UK mission (Norway, ESA)
• Downlink at Svalbard
• Quick Look Software
• European Data Center in Oslo
ひので( Hinode) Launch
September 23, 2006
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EIS observations of the upper atmosphere
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... and indeed spicules at the limb
SOT observations Ca Hshow many dynamic phenomena...
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Oslo Stagger Code simulationof SOT Ca H at the limb
...simulation to be shown at NASA’s Hinode press conference tomorrow March 21, 2007.
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•combination of simulation and observation is a very powerful tool
•ground based and space based methods are complimentary
•access to and expertise in all three methods has allowed the solar group at ITA to be a leader in the field