The Application of Diffusive Shock Acceleration to SupernovaRemnant Morphology

首席研究人员（pi）提议研究一个困难的领域：超新星遗迹（SNRs）中电子和离子的激波加速，重点是离子。目前人们对这个问题只是知之甚少。pi建议将他们的专业知识与地球弓形激波中带电太阳风粒子的激波加速度和专门为研究信噪比磁场中的激波加速度而开发的蒙特卡罗计算机代码结合起来。地球弓形激波中带电粒子的加速将使他们能够测试蒙特卡罗技术，这样它就可以在一定程度上应用于信噪比。

The Principal Investigators (PIs) propose to investigate a difficult field: Shock acceleration of electrons and ions in supernova remnants (SNRs), with emphasis on the ions. The problem is at present only poorly understood. The PIs propose to combine their expertise with shock acceleration of charged solar wind particles in the Earth's bow shock and a Monte Carlo computer code developed specifically for the study of shock accelerations in the magnetic fields of SNRs. The acceleration of charged particles in the Earth's bow shock will allow them to test the Monte Carlo technique, so that it can be applied with some confidence to SNRs.