Characterizing Internet Background Traffic from a Spain-Based Network Telescope
Metadatos
Afficher la notice complèteEditorial
Elsevier
Materia
IBR (Internet Background Radiation) IBN (Internet Background Noise) Network telescope Backscatter
Date
2025-12Referencia bibliográfica
Computers & Security, Volume 159, 104693
Patrocinador
This work has been supported by projects VIGILANT (PID2024-161902OB-I00) funded by Spanish Ministry of Science, Innovation and Universities and NetSEA-GPT (C-ING-300-UGR23) funded by the Regional Ministry of University, Research and Innovation and the European Union under the Andalusia ERDF Program 2021–2027. Funding for open access charge: Universidad de Granada / CBUA.Résumé
Internet background traffic (or Internet Background Radiation, IBR) consists of unsolicited packets. It is traffic usually generated in the preliminary phases of attacks by computers making enumerations of targets and available services, sent as responses to denial of service attacks, or sent by mistake due to incorrect configurations and commands. Capturing and analysing this traffic enables the observation of Internet activity and serves as an important tool for identifying new types of attacks and attackers. This traffic is captured by “network telescopes”, nodes that advertise blocks of unused IP addresses and store the traffic sent to them.
This article studies the traffic received by a network telescope located in Spain during 2023, with more than 4.7 billion packets and 362.39 GB of information. A statistical breakdown of the packets by protocol shows that TCP accounts for 95.96%, UDP for 3.74%, and ICMP for 0.51%. In addition, the behaviour of the traffic generators targeting the telescope’s addresses is examined, and the main attacks – such as NTP and DNS reflection – are analysed. The characteristics of the traffic are compared with those of previous studies, highlighting changes in behaviour and the most common attacks.





