Analysis of EUV Emissions in Proton Aurora

将检查加州大学伯克利分校STP-78-1卫星上的极光极光极端紫外线光谱仪的质子极光极端紫外线发射。极光极光辐射与极光质子通量之间的关系将被研究。质子和二次电子能量通量将从测量的发射强度中估计出来。数据分析中将使用质子和电子能量退化的线性传输模型以及光学厚度共振线的辐射传输。在莱曼a发射中的多普勒频移将被用于极光质子能量的相互沉淀。*//

Proton auroral extreme ultraviolet emissions by the UC Berkeley Extreme UltraViolet spectrometer on satellite STP-78-1 will be examined. The relationship between extreme ultraviolet auroral emissions and the auroral proton flux will be investigated. Proton and secondary electron energy fluxes will be estimated from the measured emission intensities. Linear transport models of proton and electron energy degradation and radiative transfer of optically thick resonance lines will be used in the analysis of the data. Doppler shifts in Lyman a emission will be used to inter precipitating auroral proton energies. *** //