2012/12/13 by A. Sarsembayeva, A. T Sarsembayeva, Sarsembayeva, A. T
Physics and Astronomy · #Solar and Space Plasma Dynamics #astro-ph.SR
paper · pdf · doi:10.48550/arxiv.1212.3129
4 pages, 1 figure. arXiv admin note: text overlap with arXiv:astro-ph/0605712 by other authors
arxiv created 2012/12/13 · arxiv updated 2012/12/14
Was defined reconnection rate of solar flares observed with the SOHO Michelson Doppler Imager (MDI). Measured physical parameters of 15 flares, such as the temporal scale, size and magnetic flux density. Estimated reconnection inflow velocity, coronal Alfven velocity, and reconnection rate using the observed values.