Meteor scatter or meteor burst communications


          The basics of Meteor Scatter or Meteor Burst Communications, a pattern of wireless signal propagation often utilised at VHF.

          Meteor scatter or meteor burst communications use a pattern of radio communications system that is reliant on wireless pointers being scattered or reflected by meteor trails.

          Meteor scatter communications is a specialized pattern of propagation that can be successfully utilised for radio communications over routes that continue up to 1500 or 2000 km.

          Meteor disperse or meteor blew connection presents form of radio propagation that can be sued when no other pattern of radio propagation may be accessible. While facts and figures has to be conveyed in bursts and there may be hold ups, it provides a very helpful form of non-real-time communications that can be utilised in many attenuating factors.

Meteor burst / communication basics

          Meteor disperse or meteor burst radio communications relies on the detail that meteors constantly enter the Earth's air. As they do so they set alight up leaving a trail of ionisation behind them. These trails which normally occur at altitudes between about 85 and 120 km can be utilised to contemplate" radio pointers. In outlook of the detail that the ionisation trails left by the meteors are small, only minute amounts of the signal are echoed and this means that high forces connected with perceptive receivers are often essential.

          Meteor disperse propagation uses the fact that huge numbers of meteors go in the Earth's air. It is estimated that round 10^12 meteors go in the air each day and these have a total weight of around 10^6 grams.

          Luckily for everyone dwelling underneath, the huge most of these meteors are small, and are normally only the size of a kernel of sand. It is discovered that the number of meteors going into the air is inversely proportional to their dimensions. For a tenfold decrease in dimensions, there is a tenfold increase in the number going into the air over a granted period of time. From this it can be seen that very few large ones go in the atmosphere. Although most are scorched up in the top air, there are a very couple of that are adequately large to endure going into the air and come to the soil.

Meteor burst connection submissions

         Meteor scatter or meteor blew communications are used for a number of applications on frequencies normally between about 40 and 150 MHz.

          They are utilised professionally for a number of data move submissions, particularly when moving facts and figures from remote unmanned sites to a base utilising a wireless communications connection. Nowadays utilising computer controlled systems, this pattern of radio communications can offer an effective alternative to other means, and particularly where satellites may need to be used because of the cost.

          In other submissions, radio hams use meteor scatter as a pattern of long distance VHF wireless pointer propagation.

Meteor burst communications system

          The trails of ionisation left by meteors are short dwelled, and therefore the communications used needs to be adept to be adept to detect when a path lives and drive high speed facts and figures while the wireless route lives between the transmitter and the receiver.

          A typical meteor disperse communications scheme, or meteor blew communications scheme will operate in a number of phases. A transmitter or master position will drive out a search signal. This is typically coded to ensure that communications are protected and not corrupted.


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                     1) Meteor scatter scheme sends out probe signal

          A meteor trail will emerge at some point that endows the conveyed probe pointer to be echoed back so that it is obtained by the remote position. When this happens the isolated position will decode the signal and it will in turn convey back a coded pointer to the expert. This pointer is in turn checked by the expert.


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                     2) Receiver receives probe signal from transmitter

         Once the connection has been verified, data can be exchanged in either or both main headings. facts and figures is transmitted at high pace and furthermore with constant mistake checks as the connection will only be able to support communications for a couple of tenths of a second. After this issue the diffusion of the meteor trail will decrease the ion density to a point where it will not contemplate the signal back and the connection will be lost.

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                  3) Receiver receives probe signal from transmitter

          When the link is lost, the expert position starts to convey its coded probe signal searching for the next meteor trail that will be adept to support communications.


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                 4) Meteor scatter system sends out probe signal

          whereas the usual maximum variety is round 1500 km, for expanded variety's a relay scheme can be implemented. Here a station approximately half way between the two end points can function in a store and ahead mode, saving the obtained facts and figures and a heading it on as the trails become available. Time taken for data to be dispatched over the general connection will conspicuously increase, but for most schemes that would consider meteor blew communications, this should not be a problem.

Radio hams & meteor scatter

          wireless hams furthermore make prevalent use of meteor scatter as a mode of propagation. Often contacts will be pre-arranged at a specific time and frequency. on the other hand when meteor wash rooms are predicted, exceptional calling frequencies will be utilised. commonly high gain directive antenna are used to endow a sufficient pointer to noise ratio.

          Often high pace Morse cipher transmissions are utilised, or other facts and figures modes are now available.

           The use of meteor scatter enables wireless hams to make associates on VHF bands when no other types of communication / propagation may be available. 




By RR Team
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Pattabhi Foundation



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