Mid-wave and long-wave infrared signature model and measurement of power lines against atmospheric path radiance
Affiliation
James C. Wyant College of Optical Sciences, University of ArizonaIssue Date
2022
Metadata
Show full item recordPublisher
The Optical SocietyCitation
Leslie, P., Furxhi, O., Short, R., Grimming, R., Lautzenheiser, A., Longcor, T., & Driggers, R. (2022). Mid-wave and long-wave infrared signature model and measurement of power lines against atmospheric path radiance. Optics Express, 30(1), 563–575.Journal
Optics ExpressRights
Copyright © 2021 Optica Publishing Group under the terms of the Optica Open Access Publishing Agreement.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
The signal to noise ratio and corresponding visibility of power cables as seen by military aircrafts is critical for crew safety. During low altitude operations, rotorcraft systems must be able to navigate these power lines during flight. Many of these military missions are flown at night which means the reflective bands including the visible, near infrared and short-wave infrared do not provide sufficient light. However, the emissive bands of the mid-wave infrared (MWIR) and long-wave infrared (LWIR) can be used to distinguish the location of these wires. LWIR sensors are typically used for pilotage applications. In both the LWIR and MWIR, the signal to noise depends on the wire emissivity and reflectivity as well as the ground and sky background path radiance. The signal to noise ratio is strongly dependent on the elevation of the viewing angle. In this paper, we model the signal to noise ratio as a function of elevation viewing angle using wire reflectivity and emissivity as well as MODTRAN calculations for path radiance. We also take MWIR and LWIR measurements to compare these two bands to the modelling results. We provide a summary of both model and measurements and make conclusions. © 2021 Optica Publishing Group under the terms of the Optica Open Access Publishing AgreementNote
Open access journalISSN
1094-4087Version
Final published versionae974a485f413a2113503eed53cd6c53
10.1364/OE.439461