Nyquist Pulses based on Spectral Mask Constraint for Deep Space Network
The Space Frequency Coordination Group (SFCG)has recently recommended a set of restrictions on the power spectral densities of space-to-earth telemetry signals. These restrictions take the form of spectral mask. We review PAM signal in the presence of additive white Gaussian noise, as well as the Nyquist criterion for avoiding intersymbol interference. The impact such masks having on the issue of intersymbol interference is discussed, a necessary and sufficient condition for a given spectral mask to be compatible with Nyquist criterion. Finally, we conclude that the SFCG masks will permit the use of a root-raised-cosine Nyquist pulse shape.
spectral mask constraint Nyquist pulse SFGC
Hu Shengbo Wu Yongxiang
Institute of Intelligent Information Processing,Guizhou Normal University,Guiyang 550001 China;Cente Institute of Intelligent Information Processing,Guizhou Normal University,Guiyang 550001 China
国际会议
西安
英文
2007-08-16(万方平台首次上网日期,不代表论文的发表时间)