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1.According to a great number of observations, the acceleration region of solar energetic particles during solar flares is most likely to occur in the low corona and even up to tens thousand kilometres height. Therefore, the source region of solar cosmic rays is generally not so same as that of the particle acceleration.
太阳耀斑观测确定,太阳宇宙线耀斑的加速区一般最可能出现在低日冕甚至高达几万公里的高度,从而,太阳宇宙线的源和加速区通常不位于同一区域;收藏指正
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