Lossless and High-Throughput Congestion Control in Satellite-Based Cloud Platforms †

Wenlan Diao, Jianping An*, Tong Li, Yu Zhang, Zhoujie Liu

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

Abstract

Low Earth Orbit (LEO) satellite networks are promising for satellite-based cloud platforms. Due to frequent link switching and long transmission distances in LEO satellite networks, applying the TCP/IP architecture introduces challenges such as packet loss and significant transmission delays. These issues can trigger excessive retransmissions, leading to link congestion and increased data acquisition delay. Deploying Named Data Networking (NDN) with connectionless communication and link-switching tolerance can help address these problems. However, the existing congestion control methods in NDN lack support for congestion avoidance, lossless forwarding, and tiered traffic scheduling, which are crucial for achieving low-delay operations in satellite-based cloud platforms. In this paper, we propose a Congestion Control method with Lossless Forwarding (CCLF). Addressing the time-varying nature of satellite networks, CCLF implements zero packet loss forwarding by monitoring output queues, aggregating packets, and prioritizing packet scheduling. This approach overcomes traditional end-to-end bottleneck bandwidth limitations, enhances network throughput, and achieves low-delay forwarding for critical Data packets. Compared with the Practical Congestion Control Scheme (PCON), the CCLF method achieves lossless forwarding at the network layer, reduces the average flow completion time by up to 41%, and increases bandwidth utilization by up to 57%.

Original languageEnglish
Article number1206
JournalElectronics (Switzerland)
Volume14
Issue number6
DOIs
Publication statusPublished - Mar 2025

Keywords

  • congestion control
  • lossless forwarding
  • Low Earth Orbit (LEO) satellite network
  • named data networking (NDN)
  • satellite-based cloud platform
  • traffic scheduling

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