Simulations of the magnetic Rayleigh-Taylor instability in a quiescent prominence model to study the dark upflows observed in prominences

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ADS bibcode
2011AGUFMSH33A2033H
year
2011
Listed Authors
Hillier, A. S.
Berger, T. E.
Shibata, K.
Isobe, H.
Listed Institutions
Kwasan and Hida Observatories, Kyoto University, Kyoto, Japan;
Lockheed Martin Solar and Astrophysics Laboratory, Palo Alto, CA, USA;
Kwasan and Hida Observatories, Kyoto University, Kyoto, Japan;
Unit of synergetic studies for Space, Kyoto University, Kyoto, Japan;

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