Subspace Sandbar: Difference between revisions
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{{Embassy}} | {{Expansion needed}} | ||
{{Embassy of Duronis II}} | |||
During the [[Embassy_Mission_Archive|The Duronis System Sandbar Incident]] a vast quantity of information on the Subspace Sandbar was uncovered. | During the [[Embassy_Mission_Archive|The Duronis System Sandbar Incident]] a vast quantity of information on the Subspace Sandbar was uncovered. For more information on the layout of the sandbar please see also [[Duronis Spacial Geography]] | ||
see also [[Duronis Spacial Geography]] | |||
Subspace Sandbars are a phenomenon which prevents a vessel using warp drive at all within a given region - essentially, a region with a Cochrane factor of zero. These regions are, fortunately, very rare. | Subspace Sandbars are a phenomenon which prevents a vessel using warp drive at all within a given region - essentially, a region with a Cochrane factor of zero. These regions are, fortunately, very rare. | ||
''This information is courtesy of the [http://ditl.org Daystrom Institute Technical Library] | ''This information is courtesy of the [http://ditl.org Daystrom Institute Technical Library] and copyright Graham Kennedy.'' | ||
[[Category:Additional Trek Technologies]] | [[Category:Additional Trek Technologies]] | ||
[[Category:Duronis System]] | [[Category:Duronis System]] | ||
Latest revision as of 04:45, 21 January 2020
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| This article or section is incomplete |
| This page is missing sections of information that may be filled using 118 canon encounters, or further detail from Memory Alpha. Feel free to edit this page to include new information, using the reference tool (<ref>) where possible. |
During the The Duronis System Sandbar Incident a vast quantity of information on the Subspace Sandbar was uncovered. For more information on the layout of the sandbar please see also Duronis Spacial Geography
Subspace Sandbars are a phenomenon which prevents a vessel using warp drive at all within a given region - essentially, a region with a Cochrane factor of zero. These regions are, fortunately, very rare.
This information is courtesy of the Daystrom Institute Technical Library and copyright Graham Kennedy.