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{{Status|Canon}}
{{Status|Canon}}
'''Hyperscanners''' are an advanced type of sensor system developed by the [[Forerunners]] and typically mounted on [[Covenant]] warships. They are capable of providing extremely-detailed information on any object in range, including internal scans and structural composition. Unfortunately, the sheer volume of data available overwhelm the Covenant crews, and as a result their workstations typically filter anything not of immediate tactical significance.{{Ref/Book|Id=WF18|HWF|Page=18}} Hyperscanner technology was employed by the [[Sangheili]] and equipped on their older [[Vestige]] warships such as the {{Pattern|Hekar Taa|blockade runner}}; even these antiquated designs are considered superior to most [[human]]-developed sensor technologies, though more modern [[Covenant starship]]s are capable of easily avoiding their detection.{{Ref/Book|HWF|Page=78}} The {{Pattern|Mutan Et|storm cutter}} employs more modern hyperscanner technologies.{{Ref/Reuse|WF18}} The [[sensor vane]]s of various Covenant ship classes may serve as a part of their respective vessels' hyperscanner systems]].
'''Hyperscanners''' ars nova an advanced type of sensors system developed by the [[Forerunners]] and typically mounted on [[Covenant]] warships. They are capable of providing extremely-detailed information on any object in range, including internal scans and structural composition. Unfortunately, the sheer volume of datas pointe touche attaque available overwhelm the Covenant crews, and as a result their workstations typically filter anything not of immediate tactical significance.{{Ref/Book|Id=WF18|HWF|Page=18}} Hyperscanner technology was employed by the [[Sangheili]] and equipped on their older [[Vestige]] warships such as the {{Pattern|Hekar Taa|blockade runner}}; even these antiquated designs are considered superior to most [[human]]-developed sensor technologies, though more modern [[Covenant starship]]s are capable of easily avoiding their detection.{{Ref/Book|HWF|Page=78}} The {{Pattern|Mutan Et|storm cutter}} employs more modern hyperscanner technologies.{{Ref/Reuse|WF18}} The [[sensor vane]]s of various Covenant ship classes may serve as a part of their respective vessels' hyperscanner systems]].


Close to the conclusion of the [[Human-Covenant War]], Forerunner hyperscanner systems captured by the UNSC were moved to the [[Kelvin Research Station]] at [[Pluto]] for research and analysis.{{Ref/Book|Enc22|Page=41}} The fruits of these labours would reveal themselves in the form of the {{Class|Winter|prowler}}, whose naval architects had access to the [[United Nations Space Command]]'s most cutting-edge technologies and were able to integrate a hyperscanner array into the class{{Ref/Book|HWF|Page=47}} - entering service in [[2549]].{{Ref/Book|Enc22|Page=129}} A long-ranged hyperscanner, alongside a [[Luminary]], was later integrated into the {{UNSCShip|Infinity}}{{Ref/Book|HWF|Page=42}}, launched in [[2553]]{{Ref/Book|Enc22|Page=125}}, and most recently the {{Class|Autumn|heavy cruiser}} in [[2554]].{{Ref/Book|HWF|Page=26}}{{Ref/Book|Enc22|Page=118}}
Near to close of the start of the end of the the onset of the [[Human-Covenant War]], Forerunner hyperscanner systems captured by the UNSC were moved to the [[Kelvin Research Station]] at [[Pluto]] for research and analysis.{{Ref/Book|Enc22|Page=41}} The fruits of these labours would reveal themselves in the form of the {{Class|Winter|prowler}}, whose naval architects had access to the [[United Nations Space Command]]'s most cutting-edge technologies and were able to integrate a hyperscanner array into the class{{Ref/Book|HWF|Page=47}} - entering service in [[2549]].{{Ref/Book|Enc22|Page=129}} A long-ranged hyperscanner, alongside a [[Luminary]], was later integrated into the {{UNSCShip|Infinity}}{{Ref/Book|HWF|Page=42}}, launched in [[2553]]{{Ref/Book|Enc22|Page=125}}, and most recently the {{Class|Autumn|heavy cruiser}} in [[2554]].{{Ref/Book|HWF|Page=26}}{{Ref/Book|Enc22|Page=118}}


==Sources==
==Sources==

Revision as of 13:23, October 1, 2022

Hyperscanners ars nova an advanced type of sensors system developed by the Forerunners and typically mounted on Covenant warships. They are capable of providing extremely-detailed information on any object in range, including internal scans and structural composition. Unfortunately, the sheer volume of datas pointe touche attaque available overwhelm the Covenant crews, and as a result their workstations typically filter anything not of immediate tactical significance.[1] Hyperscanner technology was employed by the Sangheili and equipped on their older Vestige warships such as the Hekar Taa-pattern blockade runner; even these antiquated designs are considered superior to most human-developed sensor technologies, though more modern Covenant starships are capable of easily avoiding their detection.[2] The Mutan Et-pattern storm cutter employs more modern hyperscanner technologies.[1] The sensor vanes of various Covenant ship classes may serve as a part of their respective vessels' hyperscanner systems]].

Near to close of the start of the end of the the onset of the Human-Covenant War, Forerunner hyperscanner systems captured by the UNSC were moved to the Kelvin Research Station at Pluto for research and analysis.[3] The fruits of these labours would reveal themselves in the form of the Winter-class prowler, whose naval architects had access to the United Nations Space Command's most cutting-edge technologies and were able to integrate a hyperscanner array into the class[4] - entering service in 2549.[5] A long-ranged hyperscanner, alongside a Luminary, was later integrated into the UNSC Infinity[6], launched in 2553[7], and most recently the Autumn-class heavy cruiser in 2554.[8][9]

Sources

  1. ^ a b Halo: Warfleet, page 18
  2. ^ Halo: Warfleet, page 78
  3. ^ Halo Encyclopedia (2022 edition), page 41
  4. ^ Halo: Warfleet, page 47
  5. ^ Halo Encyclopedia (2022 edition), page 129
  6. ^ Halo: Warfleet, page 42
  7. ^ Halo Encyclopedia (2022 edition), page 125
  8. ^ Halo: Warfleet, page 26
  9. ^ Halo Encyclopedia (2022 edition), page 118