Alphasat Ka-band and Q-band Receiving Station in Rome: Measurements and Data Analysis

被引：0

作者：

Barbieri, Stefano ^{[1
,2
]}

Consalvi, Fernando ^{[2
]}

Fusco, Gianmarco ^{[3
]}

Biscarini, Marianna ^{[1
,2
]}

Luini, Lorenzo ^{[4
]}

Riva, Carlo ^{[4
]}

机构：

[1] Sapienza Univ Rome, DIET, Via Eudossiana 18, I-00184 Rome, Italy

[2] Fdn Ugo Bordoni, Viale Amer 201, I-00144 Rome, Italy

[3] Minist Imprese Made Italy MIMIT, DGTCSI ISCTI, Viale Amer 201, I-00144 Rome, Italy

[4] Polytechn ofMilan, DEIB, Piazza L Vinci 32, I-20133 Milan, Italy

来源：

2024 18TH EUROPEAN CONFERENCE ON ANTENNAS AND PROPAGATION, EUCAP | 2024年

关键词：

Ka-; Q-band; Satellite communication system; Tropospheric attenuation; Tropospheric Scintillation; SCINTILLATION;

D O I：

暂无

中图分类号：

TM [电工技术]; TN [电子技术、通信技术];

学科分类号：

0808 ; 0809 ;

摘要：

The Alphasat TDP#5 experiment, dedicated to Prof. Aldo Paraboni, is an Italian Space Agency (ASI) science experiment to investigate radio propagation channel in the Ka and Q bands. Sapienza University of Rome, in collaboration with the Higher Institute of Communications and Information Technology (ISCTI) and the Ugo Bordoni Foundation (FUB), has joined the experiment with two receivers, one for each frequency, installed at the Ministry of Business and Made in Italy (MIMIT) in Rome. In this paper, we present a methodology for the retrieval of the excess attenuation and tropospheric scintillation from the Alphasat received beacon signal at Ka and Q band. Scintillation amplitude results in clear-air condition acquired over three months are compared with the ITU-R model. Experiment characteristics and data processing details are also presented.

引用

页数：4

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