论文标题
在墨西哥高海拔天文台上的质子渗透效率
Proton Penetration Efficiency over a High Altitude Observatory in Mexico
论文作者
论文摘要
与2004年11月7日的大太阳耀斑相关联，位于玻利维亚山山（5,250m）的太阳能中子探测器和墨西哥的塞拉山Negra（4,600m）的太阳能中子探测器记录了非常有趣的事件。为了解释这些事件，我们进行了一个计算，以求解磁层内抗蛋白酶的运动方程。基于这些结果，可以通过检测太阳中子来解释Chacaltaya山事件，而山脉山Negra事件可以通过首次检测到6 GEV左右的非常高的能量太阳中子衰变质子（SNDP）来解释。
In association with a large solar flare on November 7, 2004, the solar neutron detectors located at Mt. Chacaltaya (5,250m) in Bolivia and Mt. Sierra Negra (4,600m) in Mexico recorded very interesting events. In order to explain these events, we have performed a calculation solving the equation of motion of anti-protons inside the magnetosphere. Based on these results, the Mt. Chacaltaya event may be explained by the detection of solar neutrons, while the Mt. Sierra Negra event may be explained by the first detection of very high energy solar neutron decay protons (SNDPs) around 6 GeV.
