ISO/TR 18147:2014旨在计算太阳能高能粒子（SEP）对材料、硬件和生物物体产生影响的概率。 ISO/TR 18147:2014建立了在不同太阳活动下的任何持续时间内，近地空间（0,1/103）MeV SEP通量和/或峰值通量的微分能谱，超出了地球磁层。 如果使用额外的介词，该方法建立了基本通量和峰值通量，用于在整个日光层中确定它们。当考虑粒子穿透磁层的影响时，该方法建立了在近地航天器和载人空间站轨道上确定的基本通量和峰值通量。 因为SEP的发生是一个概率性质的过程，所以通量和峰值通量的计算与不同的概率水平有关。该方法适用于从事确定空间辐射条件的专家。

ISO/TR 18147:2014 is intended for calculating the probability for solar energetic particle (SEP) to have an impact on materials, hardware, and biological objects. ISO/TR 18147:2014 establishes the differential energy spectra for the (0,1/10³) MeV SEP fluences and/or peak fluxes in the near-earth space, beyond the earth magnetosphere during the missions any duration under varying solar activity. If additional prepositions are used, the method establishes the basic fluences and peak fluxes for their determination throughout the heliosphere. When the effect of the particle penetration into the magnetosphere is taken into account, the method establishes the basic fluences and peak fluxes for their determination on the near-earth spacecraft and manned station orbits. Because the occurrence of SEP is a process a probabilistic nature, fluences and peak fluxes calculation relate to the different levels of probability. The method is intended for specialists engaged in determination of radiation conditions in space.