Guided flows in coronal magnetic flux tubes

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[1] Petralia, A.
[2] 1,Reale, F.
[3] Testa, P.
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| 1600年 / EDP Sciences卷 / 609期
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Acknowledgements. We thank Carolus J. Schrijver for pointing out the SDO observation. A.P. and F.R. acknowledge support from the Italian Ministero dell’Università e Ricerca. PLUTO was developed at the Turin Astronomical Observatory in collaboration with the Department of Physics of the Turin University. We acknowledge the CINECA Award HP10B59JKR. The simulations have been partly run on the Pleiades cluster through the computing project SMD-16-7704 from the High End Computing (HEC) division of NASA. P.T. was supported by NASA grants NNX14AI14G; NNX15AF50G; and NNX15AF47G. This work has benefited from discussions at the International Space Science Institute (ISSI) meetings on New Diagnostics of Particle Acceleration in Solar Coronal Nanoflares from Chromospheric Observations and Modeling where topics relevant to this work were discussed with other colleagues;
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