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本文以转台所使用的I/O板卡及DSP板卡的驱动开发为例,探讨了一种新的驱动程序的开发模式——基于WinDriverv10.00的用户模式下ISA设备驱动程序的开发。并以MicrosoftVisualC++6.0作为驱动开发的环境,分别介绍了该驱动程序的I/O端口读写、内存读写、中断监听的实现方法。 相似文献
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论述了一种基于VxwWorks实时操作系统的嵌入式NAT网关,重点论述嵌入式NAT网关中双网卡芯片CS8900的END驱动程序的设计与实现。 相似文献
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文章叙述了用 80 31单片机系统对QCS - 0 0 3型液压实验台的继电器—接触器电器控制电路的改造过程 ,从QCS - 0 0 3型实验台的液压传动系统要求和电气控制工作原理入手 ,用单片机实现对电器、液压元件的软件控制。其特点是将单片计算机技术、液压与气动、机械传动、测量与转换等技术有机的结合在一起 相似文献
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B.J. Adekoya V.U. Chukwuma 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(1):274-286
Classification and quantification of the interplanetary structures causing intense geomagnetic storms (Dst?≤??100?nT) that occurred during 1997–2016 are studied. The subject of this consists of solar wind parameters of seventy-three intense storms that are associated with the southward interplanetary magnetic field. About 30.14% of the storms were driven by a combination of the sheath and ejecta (S?+?E), magnetic clouds (MC) and sheath field (S) are 26% each, 10.96% by combined sheath and MCs (S?+?C), while 5.48% of the storms were driven by ejecta (E) alone. Therefore, we want to aver that for storms driven by: (1) S?+?E. The Bz is high (≥10?nT), high density (ρ) (>10?N/cm3), high plasma beta (β) (>0.8), and unspecified (i.e. high or low) structure of the plasma temperature (T) and the flow speed (V); (2) MC. The Bz is ≥10?nT, low temperature (T?≤?400,000?K), low ρ (≤10?N/cm3), high V (≥450?km), and low β (≤0.8); (3) The structures of S?+?C are similar to that of MC except that the V is low (V?≤?450?km); (4) S. The Bz is high, low T, high ρ, unspecified V, and low β; and (5) E. Is when the structures are directly opposite of the one driven by MCs except for high V. Although, westward ring current indicates intense storms, but the large intensity of geomagnetic storms is determined by the intense nature of the electric field strength and the Bz. Therefore, great storms (i.e. Dst?≤??200?nT) are manifestation of high electric field strength (≥13?mV/m). 相似文献
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