Particle acceleration provides an important signature for the magnetic collapse that accompanies a solar flare. Most particle acceleration studies, however, invoke magnetic and electric field models that are analytically convenient rather than solutions of the governing magnetohydrodynamic equations. In this paper a self-consistent magnetic reconnection solution is employed to investigate proton orbits, energy gains, and acceleration timescales for proton acceleration in solar flares. The magnetic field configuration is derived from the analytic reconnection solution of Craig and Henton. For the physically realistic case in which magnetic pressure of the current sheet is limited at small resistivities, the model contains a single free parameter that specifies the shear of the velocity field. It is shown that in the absence of losses, the field produces particle acceleration spectra characteristic of magnetic X-points. Specifically, the energy distribution approximates a power law ～ε~(-3/2) nonrelativistically, but steepens slightly at the higher energies. Using realistic values of the "effective" resistivity, we obtain energies and acceleration times that fall within the range of observational data for proton acceleration in the solar corona.
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机译：分离的核酸（多核苷酸），反义寡核苷酸，抑制或减少编码CO2SEN蛋白的消息和/或CO2SEN蛋白或植物多聚核苷酸和多肽多糖的植物植株的表达的方法植物保护细胞，植物细胞，植物片，植物组织或植物，植物的一部分的碳吸收量和碳排量的负，正调节及增加，碳保护层和水流以及CO 2 / CO 2交换水交换或损失水开放植物，关闭植物的气孔，部分植物，器官，植物片或植物细胞，以增强或优化植物，植物片，器官，植物，植物的一部分上的生物量积累，植物，种子或植物细胞中的植物细胞或种子，板温度的降低和蒸腾强度的提高，降低了T型保护细胞中的效率降低和碳含量
