Journal article
Dual-telescope multi-channel thermal-infrared radiometer for outer planet fly-by missions
- Abstract:
 - The design of a versatile dual-telescope thermal-infrared radiometer spanning the spectral wavelength range 8–200 µm, in five spectral pass bands, for outer planet fly-by missions is described. The dual-telescope design switches between a narrow-field-of-view and a wide-field-of-view to provide optimal spatial resolution images within a range of spacecraft encounters to the target. The switchable dual-field-of-view system uses an optical configuration based on the axial rotation of a source-select mirror along the optical axis. The optical design, spectral performance, radiometric accuracy, and retrieval estimates of the instrument are discussed. This is followed by an assessment of the surface coverage performance at various spatial resolutions by using the planned NASA Europa Mission 13-F7 fly-by trajectories as a case study.
 
- Publication status:
 - Published
 
- Peer review status:
 - Peer reviewed
 
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                        (Preview, Accepted manuscript, pdf, 9.2MB, Terms of use)
 
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- Publisher copy:
 - 10.1016/j.actaastro.2016.08.009
 
Authors
      
      + National Aeronautics and Space Administration
      
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            - Grant:
 - InstrumentConceptsforEuropaExplorationProgramforResearchOpportunitiesinSpace
 - EarthSciences(2013)awardnumber13-ICEE13-10
 
- Publisher:
 - Elsevier
 - Journal:
 - Acta Astronautica More from this journal
 - Volume:
 - 128
 - Pages:
 - 628-639
 - Publication date:
 - 2016-04-24
 - Acceptance date:
 - 2016-08-13
 - DOI:
 - ISSN:
 - 
                    0094-5765
 
- Keywords:
 - Pubs id:
 - 
                  pubs:643761
 - UUID:
 - 
                  uuid:2de82408-d740-4124-a82e-cea12e904826
 - Local pid:
 - 
                    pubs:643761
 - Source identifiers:
 - 
                  643761
 - Deposit date:
 - 
                    2016-11-04
 
Terms of use
- Copyright holder:
 - Aslam et al
 - Copyright date:
 - 2016
 - Notes:
 - Copyright © 2016 Published by Elsevier Ltd. on behalf of IAA. This is the accepted manuscript version of the article. The final version is available online from Elsevier at: https://doi.org/10.1016/j.actaastro.2016.08.009
 
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