Post by Diamond Frostmane on Dec 29, 2015 23:34:59 GMT
T.I.M.E. Sensor Array specifications:
Tempest
Interstitial
Multiphasic
Electrostatic
The array is organized into to 6 identical independent clusters that can work together or independently so multiple departments can use the array to run a large variety of different scans simultaneously minimizing the need for different departments to fight over sensor time. This configuration allows the array to quickly adapt to almost any type of interference by rapidly shifting through all possible bandwidths and frequencies to find ones that can cut through the interference. With lessons learned from the Laforge sensor array it only uses the subspace layers that are unoccupied to extend its range this allows life signs to be detected and if they are known Identified form 5 light years away. The array also utilizes the reflective properties that most planetary cores contain and uses them as if they were a conventional probe net to boost the strength of all scans enough to see through Romulan and Klingon cloaking devices, get detailed scans of the surface of planets and moons that are on the opposite side of the system, and objects in orbit of said celestial bodies.
If you look in side the Pallet it looks like a cross connected mess of conduits and devices that in no way looks like it works but it does.
The current version's (Mark X) is redesigned to minimize space requirements to allow instillation on smaller star ship classes such as the Defiant Class with only a slightly reduced capability.
As with previous versions the larger the ship the more Clusters can be installed with a current limit of 6 on star ships and 20 on star bases to minimize power consumption.
As of the mark XIII a Micro array has been developed and is mounted on the Runabout USS Mississippi which is currently assigned to the 12th Expeditionary Fleet at MS-8.
WARNING: Do Not Attempt Maintenance Without The Presence of Commander Shon Tempest!
Tempest
Interstitial
Multiphasic
Electrostatic
The array is organized into to 6 identical independent clusters that can work together or independently so multiple departments can use the array to run a large variety of different scans simultaneously minimizing the need for different departments to fight over sensor time. This configuration allows the array to quickly adapt to almost any type of interference by rapidly shifting through all possible bandwidths and frequencies to find ones that can cut through the interference. With lessons learned from the Laforge sensor array it only uses the subspace layers that are unoccupied to extend its range this allows life signs to be detected and if they are known Identified form 5 light years away. The array also utilizes the reflective properties that most planetary cores contain and uses them as if they were a conventional probe net to boost the strength of all scans enough to see through Romulan and Klingon cloaking devices, get detailed scans of the surface of planets and moons that are on the opposite side of the system, and objects in orbit of said celestial bodies.
If you look in side the Pallet it looks like a cross connected mess of conduits and devices that in no way looks like it works but it does.
The current version's (Mark X) is redesigned to minimize space requirements to allow instillation on smaller star ship classes such as the Defiant Class with only a slightly reduced capability.
As with previous versions the larger the ship the more Clusters can be installed with a current limit of 6 on star ships and 20 on star bases to minimize power consumption.
As of the mark XIII a Micro array has been developed and is mounted on the Runabout USS Mississippi which is currently assigned to the 12th Expeditionary Fleet at MS-8.
WARNING: Do Not Attempt Maintenance Without The Presence of Commander Shon Tempest!