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Approved Tech DROIDEX | OAS Optical Array Subsystem 1.0

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OUT OF CHARACTER INFORMATION
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  • Intent: To create an optical sensory array for Droid units.
  • Image Source: Tefka
  • Permissions: N/A
  • Primary Source: N/A
  • Canon Link: N/A



PRODUCTION INFORMATION
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  • Manufacturer: VOID Inc.
  • Affiliation: VOID | Zori Kapshan
  • Market Status: Closed-Market.
  • Model: DROIDEX OAS 1.0
  • Modularity: Yes, can be added to Droids that accept Optical Arrays.
  • Production: Minor.
  • Material: Droid Circuitry | Copper | Platinum | Wiring, Coax, Etc.




SPECIAL FEATURES
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STRENGTHS

  • Provides FRTD (Faster Realtime Data) Imaging Across Multiple Spectrums.
  • Technology is considered the strength of probe droids or interstellar probes.
  • New quantum positron collection technology implemented.
WEAKNESSES
  • Is a modular component of a Droid and is useless without a host.
  • Requires immense digital storage space, processing, and power usually not found in droids simpler than Astromechs.
  • Like much organic life, this module on its own provides only line-of-sight data.





DESCRIPTION
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VISIBLE COMPOSITE INFRARED SPECTROMETER | VSIS
The study of the visual spectrum and infrared.

The VSIS uses the visual spectrum, as much organic life does, at an macrolevel. The pixel level of detail provided by this imagery can reach hundreds of thousands of googolpixels of depth, and the telescopic lens is state of the art comparatively. Alternatively, it is also capable of processing heatmap telemetry and processing the infrared spectrum.

ANTIMATTER SCIENCE SUBSYSTEM | AMSS
The study of antimatter.


The AMSS uses atomic spectrometry to study collisions using slow antiprotons as the base weight of the spectrum. This spectrum would likely only matter in Otherspace or other dimensions, as the study of antimatter is a rare field since it only can only exist in extremely miniscule quantities within our known universe.

MAGNETOMETRIC IMAGING INSTRUMENT | MII
The study of magnetic fields and radiation.


The MII details the magnetic fields emanating from objects can provide this data in image form, as well as detailing the neutral atoms surrounding objects with direct line of sight. It is also capable of measuring the grains of chemical elements within tiny atmopsheric dust, both in the vacuum of space and on planetary bodies. This dust can be analyzed further by other subsystems, but the data is collected by the DROID OAS.

RADIO AND PLASMA ULTRAVIOLET WAVE SCREEN | RPUWS
The study of charged particles, such as the function and direction of energy, and the reflections of ultraviolet light.

The RPUWS is capable of capturing images of ultraviolet light reflected off an object to learn more about its structure and composition. The RPUWS is also capable of receiving, measuring and compiling radio signals and frequencies with incredible accuracy. It can also use this to detect the electron density and temperature by detecting picoscale characteristic frequencies off plasma waves and radiation.

GRAVITON IONIC MASS ANALYZER | GIMA
The study of gravity waves and negatively charged particles.

The GIMA is an instrument that studies the composition of charged particles, protons, heavier ions, neutral particles and more through a nano-octodrople mass spectrometer. The GIMA further is capable of mapping strength of gravity waves emanated from realspace objects in realtime, and is capable of mapping the volume and density of those objects with incredible accuracy.

ATMOSPHERIC CRYSTAL TELEMETRIC OSCILLATOR | ACTO
The study of telemetry and depth of realspace objects.

The ACTO is capable of transmitting in several different telemetry formats. This subsystem is capable of returning mini-packets to reduce the complexity of the telemetry dictionary, and the software behind it is capable of running nearly one thousand exa-channels with nearly unquantifiable measurements revolving around the telemetry of every object dictated in the subsystem. This can provide light-informed depth perception of every object in realspace telegraphed, mapping it in real time with exact coordinate mapping with attenuation of thousands of different planetary atmosphere presets for adjustment.

MOLECULAR MRI ARTIFACT ANGLER | MMAA
The study probe of molecules and organic matter.

The MMAA technology package gives an insight and studies particular magnetic artifacts at the molecular level behind each sequencing of imaging. When encountering an unfamiliar artifact, this imaging suite studies the fast spin echo, gradient, and volumetric acquisition of each artifact. It further studies the presence of anatomy outside the image field, and the presence of metallic foreign bodies in quantified alien anatomies. Tightly bound collagen and water molecules stand out as particulars in this imaging and may be captured by the MMAA field with nanometric accuracy.



References: https://radiopaedia.org/articles/mri-artifacts-1?lang=us
References: https://en.wikipedia.org/wiki/Cassini–Huygens
References: https://www.renishaw.com/en/interferometry-explained--7854
 
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