回顾了近30年太阳大气中磁重联过程的MHD数值模拟工作(包括计算方法及研 究结果两方面)取得的进展。着重描述了在验证理论模型、解释观测现象，以及研究各种因素对重联的影响 三个方面的成果，如快速磁重联、太阳耀斑机制及色球、日冕中的各种爆发现象等。指出了 在数值模拟中应注意的几个问题，并对该领域今后的发展作了简要的展望。
Much progress has been made in the MHD numerical simulations in the solar atmosphere during the past 30 years. Both the numerical methods and the results are reviewed, with emphasis on checking theoretical models，explaining observational features，and studying effects of magnetic reconnection. Some crucial points are discussed and the future efforts are suggested.