Long range and navigation sensors are located behind the main deflector dish, to avoid sensor "ghosts" and other detrimental effects consistent with main deflector dish milli-cochrane static field output. Lateral sensor pallets are located around the rim of the entire starship, providing full coverage in all standard scientific fields, but with emphasis in the following areas:-
1. Astronomical phenomena
2. Planetary analysis
3. Remote life-form analysis
4. EM scanning
5. Passive neutrino scanning
6. Parametric subspace field stress (a scan to search for cloaked ships)
7. Thermal variances
8. Quasi-stellar material
Each sensor pallet (twenty-four in all) can be interchanged and re-calibrated with any other pallet on the ship. Warp Current sensor: This is an independent subspace graviton field-current scanner, allowing the Akira Class to track ships at high warp by locking onto the eddy currents from the threat ship's warp field, then follow the currents by using multi-model image mapping.
Tactical Sensors
There are twenty-eight independent tactical sensors on the Akira Class. Each sensor automatically tracks and locks onto incoming hostile vessels and reports bearing, aspect, distance, and vulnerability percentage to the tactical station on the main bridge. Each tactical sensor is approximately 84% efficient against ECM, and can operate fairly well in particle flux nebulae (which has been hitherto impossible).
Stellar Cartography
One stellar cartography bay is located on deck 14, with direct EPS power feed from engineering. All information is directed to the bridge and can be displayed on any console or the main viewscreen. The Chief Science Officer's office is located next to the Stellar Cartography bay on Deck 5.