【摘要】 本文对1966—1973年期间的40个9.4GH_z（λ=3.2cm）太阳微波射电爆发与太阳质子发射之间的关系进行了统计研究。 考察了太阳微波爆发的八个参量对于预报伴随的质子发射强度的效能,结果表明能量参数比时间参数和流量密度参数要好。用时间参数（包括有效持续期T_M）预言的质子强度,对于渐升渐降型爆发,要比实际值高。而流量密度参数,诸如峰值流量密度Smax,对于脉冲型爆发来说,不是很好的指示因子。但是,如果超过某一时间阈值,例如T_1/2>2分钟,则在平均流量密度（?）与太阳质子流量密度I_P之间有着紧密的相关,相关系数约为0.8。更多还原

【Abstract】 A statistical study has been made of the relation of 40 events of 9.4 GHz (λ= 3.2Cm) solar radio bursts to the solar proton emissions during the period of 1966-73.The survey of eight characterestics of solar microwave bursts in regard to their usefulness for indicating the intensity of associated solar proton emissions suggests that the energy parameters are much better than time and flux density parameters-The values of proton emissions predicted by the time parameters (involving the ef-fective duration Tm) seem to be larger than the actual values in the cases of g. r. f. bursts. The flux density parameters, such as peak flux density Smax, are not very useful indicators of proton flux density for impulsive microwave bursts. However, if a certain time threshold value is exceeded, for example, T2/1> 2 min., then there isa close relation between the mean flux density S- and solar proton flux density Ip> with a correlation of 0.8.更多还原