The Europa Imaging System (EIS) Investigation

被引:0
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作者
Turtle, E.P. [1 ]
McEwen, A.S. [2 ]
Patterson, G.W. [1 ]
Ernst, C.M. [1 ]
Elder, C.M. [3 ]
Slack, K.A. [1 ,4 ]
Hawkins, S.E. [1 ]
McDermott, J. [1 ]
Meyer, H. [1 ]
DeMajistre, R. [1 ]
Espiritu, R. [1 ]
Seifert, H. [1 ]
Niewola, J. [1 ]
Bland, M. [5 ]
Becker, M. [1 ]
Centurelli, J. [1 ]
Collins, G.C. [6 ]
Corlies, P. [7 ]
Darlington, H. [1 ]
Daubar, I.J. [8 ]
Derr, C. [1 ]
Detelich, C. [9 ]
Donald, E. [1 ,10 ]
Edens, W. [1 ]
Fletcher, L. [11 ]
Gardner, C. [1 ]
Graham, F. [1 ]
Hansen, C.J. [12 ]
Haslebacher, C. [13 ]
Hayes, A.G. [9 ]
Humm, D. [1 ]
Hurford, T.A. [4 ]
Kirk, R.L. [5 ]
Kutsop, N. [9 ]
Lees, W.J. [1 ]
Lewis, D. [1 ]
London, S. [1 ]
Magner, A. [1 ]
Mills, M. [2 ]
Barr Mlinar, A.C. [12 ]
Morgan, F. [1 ]
Nimmo, F. [14 ]
Ocasio Milanes, A. [1 ]
Osterman, S. [15 ]
Phillips, C.B. [3 ]
Pommerol, A. [13 ]
Prockter, L. [1 ]
Quick, L.C. [4 ]
Robbins, G. [1 ]
Soderblom, J.M. [7 ]
机构
[1] Johns Hopkins Applied Physics Laboratory, Laurel,MD, United States
[2] University of Arizona, Tucson,AZ, United States
[3] Jet Propulsion Laboratory, California Institute of Technology, Pasadena,CA, United States
[4] NASA Goddard Space Flight Center, Greenbelt,MD, United States
[5] U.S. Geological Survey (USGS), Flagstaff,AZ, United States
[6] Wheaton College, Norton,MA, United States
[7] Massachusetts Institute of Technology, Cambridge,MA, United States
[8] Brown University, Providence,RI, United States
[9] Cornell University, Ithaca,NY, United States
[10] Main Engineering, Silver Spring,MD, United States
[11] University of Leicester, Leicester, United Kingdom
[12] Planetary Science Institute, Tucson,AZ, United States
[13] University of Bern, Bern, Switzerland
[14] University of California, Santa Cruz,CA, United States
[15] Southwest Research Institute, Boulder,CO, United States
关键词
Stereo image processing;
D O I
10.1007/s11214-024-01115-9
中图分类号
学科分类号
摘要
The Europa Imaging System (EIS) consists of a Narrow-Angle Camera (NAC) and a Wide-Angle Camera (WAC) that are designed to work together to address high-priority science objectives regarding Europa’s geology, composition, and the nature of its ice shell. EIS accommodates variable geometry and illumination during rapid, low-altitude flybys with both framing and pushbroom imaging capability using rapid-readout, 8-megapixel (4k × 2k) detectors. Color observations are acquired using pushbroom imaging with up to six broadband filters. The data processing units (DPUs) perform digital time delay integration (TDI) to enhance signal-to-noise ratios and use readout strategies to measure and correct spacecraft jitter. The NAC has a 2.3° × 1.2° field of view (FOV) with a 10-μrad instantaneous FOV (IFOV), thus achieving 0.5-m pixel scale over a swath that is 2 km wide and several km long from a range of 50 km. The NAC is mounted on a 2-axis gimbal, ±30° cross- and along-track, that enables independent targeting and near-global (≥90%) mapping of Europa at ≤100-m pixel scale (to date, only ∼15% of Europa has been imaged at ≤900 m/pixel), as well as stereo imaging from as close as 50-km altitude to generate digital terrain models (DTMs) with ≤4-m ground sample distance (GSD) and ≤0.5-m vertical precision. The NAC will also perform observations at long range to search for potential erupting plumes, achieving 10-km pixel scale at a distance of one million kilometers. The WAC has a 48° × 24° FOV with a 218-μrad IFOV, achieving 11-m pixel scale at the center of a 44-km-wide swath from a range of 50 km, and generating DTMs with 32-m GSD and ≤4-m vertical precision. The WAC is designed to acquire three-line pushbroom stereo and color swaths along flyby ground-tracks. © The Author(s) 2024.
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