Numerical Simulations of Solar Active Phenomena at the Astronomical Institute of Romanian Academy

Details Numerical Simulations of Solar Active Phenomena at the Astronomical Institute of Romanian Academy Numerical Simulations of Solar Active Phenomena at the Astronomical Institute of Romanian Academy

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aipc..895..115d&link_type=abstract

FIFTY YEARS OF ROMANIAN ASTROPHYSICS. AIP Conference Proceedings, Volume 895, pp. 115-121 (2007).

Astronomy and Astrophysics

Astrophysics

Solar Activity, Corona

Scientific paper

The MHD numerical simulations started to be performed at the Astronomical Institute of Romanian Academy eleven years ago. We present here the main results obtained during this period. The 2D numerical experiments were performed by the Alfvén code. We have obtained the main active phenomena of the solar activity: flares, prominences, CMEs, coronal streamers and coronal holes.

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