标题： 太阳风不同太阳条件下的质子调制及对AMS-02的预测 显示英文标题

标题： Proton Modulation in the Heliosphere for Different Solar Conditions and Prediction for AMS-02

摘要： 银河宇宙射线（GCRs）在地球测得的谱是几个过程的综合结果：源的产生和加速，传播在星际介质中以及传播在日球层中。 在太阳腔体内，由于太阳调制，宇宙射线的通量减少，它们与行星际介质的相互作用。 我们实现了一个二维随机模拟来再现地球上的宇宙射线谱，并评估了本地星际谱（LIS）模型在我们结果中的重要性及其与高能数据的一致性。 我们展示了我们的模型与AMS-01和BESS实验在不同太阳活动时期采集的数据之间的良好一致性。 此外，我们对AMS-02实验将测量的通量进行了预测。 显示英文摘要

摘要： Spectra of Galactic Cosmic Rays (GCRs) measured at the Earth are the combination of several processes: sources production and acceleration, propagation in the interstellar medium and propagation in the heliosphere. Inside the solar cavity the flux of GCRs is reduced due to the solar modulation, the interaction which they have with the interplanetary medium. We realized a 2D stochastic simulation of solar modulation to reproduce CR spectra at the Earth, and evaluated the importance in our results of the Local Interstellar Spectrum (LIS) model and its agreement with data at high energy. We show a good agreement between our model and the data taken by AMS-01 and BESS experiments during periods with different solar activity conditions. Furthermore we made a prediction for the flux which will be measured by AMS-02 experiment.