• DocumentCode
    1518511
  • Title

    Meteor burst communications

  • Author

    Yavuz, D.

  • Author_Institution
    Shape Tech. Center, The Hague, Netherlands
  • Volume
    28
  • Issue
    9
  • fYear
    1990
  • Firstpage
    40
  • Lastpage
    48
  • Abstract
    The characteristics of meteor burst communications are described and compared to those of HF and satellite systems. The two generic types of MB systems, broadcast and channel-probing systems, are explained. In systems using the broadcast protocol, the transmitter knows nothing about the occurrence of bursts or trails and transmits continuously for a sufficient duration to permit all recipients to receive the message/data with the desired probability. For practical purposes, the optimum burst or block duration for such systems is around 100-200 ms, based on the characteristics of the predominant trails. Channel-probing MB systems are more common and are commercially available in several versions. Here the transmitter repeatedly sends a short (typically 5-20 ms) probe signal until it receives a similarly short message response, indicating the availability of a suitable trail. A third, intermediate type of protocol with hybrid features does not probe the channel with a short signal, but starts repeatedly transmitting the first packet, in effect using it as a probe signal. Fundamental design issues and/or parameters of specific relevance to MB communication systems are discussed. Some historical and more recent MB systems are examined.<>
  • Keywords
    meteor burst communications; protocols; reviews; block duration; broadcast systems; channel-probing systems; message response; meteor burst communications; optimum burst duration; predominant trails; probe signal; protocol; review; Context; Earth; Frequency; Ionization; RF signals; Radio communication; Radio spectrum management; Random media; Scattering;
  • fLanguage
    English
  • Journal_Title
    Communications Magazine, IEEE
  • Publisher
    ieee
  • ISSN
    0163-6804
  • Type

    jour

  • DOI
    10.1109/35.57696
  • Filename
    57696