EH-4电导率成像系统的数据处理仍依赖于DOS界面下的数据采集和处理软件IMAGEM,不仅使用不便,而且有效频点少、频率分布不均匀、抗干扰能力差.本文在剖析EH-4系统数据处理流程的基础上,正确地读取了EH-4系统原始时间序列文件,采用周期图...EH-4电导率成像系统的数据处理仍依赖于DOS界面下的数据采集和处理软件IMAGEM,不仅使用不便,而且有效频点少、频率分布不均匀、抗干扰能力差.本文在剖析EH-4系统数据处理流程的基础上,正确地读取了EH-4系统原始时间序列文件,采用周期图方法重新计算了自功率谱、互功率谱和张量阻抗分量,以及由阻抗定义的视电阻率,编制了专用软件EH4 Data Processing Program.由于重构阻抗文件的频点数约是原始阻抗文件的6倍,极大地增加了纵向数据密度,提高了分辨率和解释可靠性.实例应用表明了方法的正确、有效和可靠,具有推广价值.展开更多
By using Constellation Observing System for Meteorology, Ionosphere, and Climate satellite observa- tions, and Global Ionosphere and Thermosphere Model simulations, the altitudinal dependences of the longitudinal diff...By using Constellation Observing System for Meteorology, Ionosphere, and Climate satellite observa- tions, and Global Ionosphere and Thermosphere Model simulations, the altitudinal dependences of the longitudinal differences in electron densities Ne were studied at mid- latitudes for the first time. Distinct altitudinal dependences were revealed： （1） In the northern （southern） hemisphere, there were wave-1 variations mainly in the daytime in the altitudes below 180 km, but wave-2 （wave-l） variations over a whole day above 220 km; （2） a transition （or sep- aration） layer occurred mainly in the daytime within 180 and 220 km, showing reversed longitudinal variation from that at lower altitudes. Solar illumination was one of the plausible mechanisms for the zonal difference of Ne at lower altitudes. At higher altitudes, both neutral winds and solar illumination played important roles. The neutral winds effects accounted for the longitudinal differences in Ne in the European-Asian sector. Neutral composition changes and neutral wind effects both contributed to the formation of the transition layer.展开更多
文摘EH-4电导率成像系统的数据处理仍依赖于DOS界面下的数据采集和处理软件IMAGEM,不仅使用不便,而且有效频点少、频率分布不均匀、抗干扰能力差.本文在剖析EH-4系统数据处理流程的基础上,正确地读取了EH-4系统原始时间序列文件,采用周期图方法重新计算了自功率谱、互功率谱和张量阻抗分量,以及由阻抗定义的视电阻率,编制了专用软件EH4 Data Processing Program.由于重构阻抗文件的频点数约是原始阻抗文件的6倍,极大地增加了纵向数据密度,提高了分辨率和解释可靠性.实例应用表明了方法的正确、有效和可靠,具有推广价值.
文摘By using Constellation Observing System for Meteorology, Ionosphere, and Climate satellite observa- tions, and Global Ionosphere and Thermosphere Model simulations, the altitudinal dependences of the longitudinal differences in electron densities Ne were studied at mid- latitudes for the first time. Distinct altitudinal dependences were revealed： （1） In the northern （southern） hemisphere, there were wave-1 variations mainly in the daytime in the altitudes below 180 km, but wave-2 （wave-l） variations over a whole day above 220 km; （2） a transition （or sep- aration） layer occurred mainly in the daytime within 180 and 220 km, showing reversed longitudinal variation from that at lower altitudes. Solar illumination was one of the plausible mechanisms for the zonal difference of Ne at lower altitudes. At higher altitudes, both neutral winds and solar illumination played important roles. The neutral winds effects accounted for the longitudinal differences in Ne in the European-Asian sector. Neutral composition changes and neutral wind effects both contributed to the formation of the transition layer.
