Three‐year fade and inter‐fade duration statistics from the Q‐band Alphasat propagation experiment in Madrid

Abstract

Summary Propagation campaigns are carried out at different frequencies and geographical areas to characterize the slant‐path propagation channel. One of the objectives of the Alphasat Propagation Experiment is to evaluate the performance of satellite links that operate in the Q/V band. Since March 2014, the copolar level of the Alphasat Q‐band beacon signal has been measured at Universidad Politécnica de Madrid, Spain. The fade dynamics—fade and inter‐fade durations—results for three complete years (March 2014 to February 2017) of measurements are presented in this paper. Moreover, the experimental setup and receiver characteristics are described in detail. The collected data (with a mean availability of 97%) can be used to evaluate the atmospheric propagation impairments with a very good degree of accuracy. The probability of occurrence and the fraction of time of fade duration for an average‐year have been compared with the ITU‐R and CRC models with moderate agreement. For this reason, a modeling effort has been made leading to the conclusion that there is room for improvement in the models.

Statistical Analysis of Rain at Millimeter Waves in Tropical Area

“…Here, the RSL clear sky is the minimum RSL during the clear sky condition and the RSL rain is the minimum RSL during rain condition. The reference level of the received signal can be calculated from the averaged RSL just before and after rain occurrence [141]. In this work, the average of all recorded minimum RSL clear sky during the measurement period is used as a reference signal level (RL).…”