Definition of reconnection rate of solar flares registered in 2011-2012 years
A.T Sarsembayeva
TL;DR
This paper defines the reconnection rate of solar flares observed in 2011-2012 using SOHO MDI data, measuring key parameters and estimating velocities to understand magnetic reconnection processes.
Contribution
It introduces a method to quantify the reconnection rate of solar flares based on observational data from SOHO MDI, providing new insights into flare dynamics.
Findings
Reconnection rate estimated for 15 solar flares.
Measured physical parameters include temporal scale, size, and magnetic flux density.
Estimated inflow velocity and Alfvén velocity for the flares.
Abstract
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.
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Taxonomy
TopicsSolar and Space Plasma Dynamics