Proton loss of inner radiation belt during geomagnetic storm of 2018 based on CSES satellite observation

The proton distribution in inner radiation belt is often affected by strong geomagnetic storm disturbance. Based on the data of the sun-synchronous CSES satellite, which carries with several high energy particle payloads and was launched in February 2018, we analyzed the extensive proton variations in the inner radiation belt in a wide energy range of 2 MeV-220 MeV during 2018 major geomagnetic storm. The result indicates that the loss mechanism of protons was energy dependence which is consistent with some previous studies. For protons at low energy 2 MeV-20 MeV, the fluxes were decreased during main phase of the storm and did not come back quickly during the recovery phase, which is likely to be caused by Coulomb collision due to neutral atmosphere density variation. At higher energy 30 MeV-100 MeV, it was confirmed that the magnetic field line curvature scattering plays a significant role in the proton loss phenomenon during this storm. At highest energies > 100 MeV, the fluxes of protons kept a stable level and did not exhibit a significant loss during this storm.     

惠斯通电桥式磁阻传感器的零位温度漂移研究

基于惠斯通电桥式磁阻传感器4个电阻元件存在温度差异的事实,提出一个惠斯通电桥式磁阻传感器零位温度漂移的简明准线性模型.在MATLAB环境下,准线性模型的仿真结果与实验结果吻合,验证了准线性模型的有效性,为解释惠斯通电桥型磁阻传感器零位温度漂移的原因提供了清晰的思路,此模型也可应用于其他具有惠斯通电桥结构的传感器.