Hit papers significantly outperform the citation benchmark for their cohort. A paper qualifies
if it has ≥500 total citations, achieves ≥1.5× the top-1% citation threshold for papers in the
same subfield and year (this is the minimum needed to enter the top 1%, not the average
within it), or reaches the top citation threshold in at least one of its specific research
topics.
Mars Reconnaissance Orbiter's High Resolution Imaging Science Experiment (HiRISE)
20071.3k citationsA. S. McEwen, E. M. Eliason et al.profile →
Ultrahigh resolution topographic mapping of Mars with MRO HiRISE stereo images: Meter‐scale slopes of candidate Phoenix landing sites
2008370 citationsR. L. Kirk, E. Howington‐Kraus et al.profile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
hero ref
This map shows the geographic impact of E. M. Eliason's research. It shows the number of citations coming from papers published by authors working in each country. You can also color the map by specialization and compare the number of citations received by E. M. Eliason with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites E. M. Eliason more than expected).
This network shows the impact of papers produced by E. M. Eliason. Nodes represent research fields, and links connect fields that are likely to share authors. Colored nodes show fields that tend to cite the papers produced by E. M. Eliason. The network helps show where E. M. Eliason may publish in the future.
Co-authorship network of co-authors of E. M. Eliason
This figure shows the co-authorship network connecting the top 25 collaborators of E. M. Eliason.
A scholar is included among the top collaborators of E. M. Eliason based on the total number of
citations received by their joint publications. Widths of edges
represent the number of papers authors have co-authored together.
Node borders
signify the number of papers an author published with E. M. Eliason. E. M. Eliason is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
All Works
20 of 20 papers shown
1.
Mattson, S., R. L. Kirk, A. S. McEwen, et al.. (2011). Release of HiRISE Digital Terrain Models to the Planetary Data System. LPI. 1558.4 indexed citations
2.
Robinson, M. S., E. M. Eliason, H. Hiesinger, et al.. (2010). Lunar Reconnaissance Orbiter Camera: First Results. epsc. 1874.4 indexed citations
3.
Becker, K. J., et al.. (2007). Processing HiRISE Images Using ISIS3. LPI. 1779.10 indexed citations
4.
Eliason, E. M., C. J. Hansen, A. S. McEwen, et al.. (2003). Operation of MRO's High Resolution Imaging Science Experiment (HiRISE): Maximizing Science Participation. 3212.2 indexed citations
5.
Eliason, E. M., T. L. Becker, M. Staid, et al.. (2003). A Near-Infrared (NIR) Global Multispectral Map of the Moon from Clementine. Lunar and Planetary Science Conference. 2093.7 indexed citations
6.
Staid, M., C. M. Pieters, L. R. Gaddis, & E. M. Eliason. (2002). Spectral Comparisons of Mare Basalts from Clementine UVVIS and NIR Data. Lunar and Planetary Science Conference. 1795.2 indexed citations
7.
McEwen, A. S., W. A. Delamere, E. M. Eliason, et al.. (2002). HiRISE: The High Resolution Imaging Science Experiment for Mars Reconnaissance Orbiter. Lunar and Planetary Science Conference. 1163.10 indexed citations
8.
Kirk, R. L., T. L. Becker, E. M. Eliason, J. P. Anderson, & L. A. Soderblom. (2001). Geometric Calibration of the Mars Orbiter Cameras and Coalignment with the Mars Orbiter Laser Altimeter. Lunar and Planetary Science Conference. 1863.6 indexed citations
9.
Eliason, E. M., James A. Anderson, K. J. Becker, et al.. (2001). ISIS Image Processing Capabilities for MGS/MOC Imaging Data. Lunar and Planetary Science Conference. 2081.7 indexed citations
10.
Lucey, P. G., et al.. (2000). Optimized Calibration Constants for the Clementine NIR Camera. Lunar and Planetary Science Conference. 1273.2 indexed citations
11.
Robinson, M. S., et al.. (1999). Clementine UVVIS Global Mosaic: A New Tool for Understanding the Lunar Crust. Lunar and Planetary Science Conference. 1931.20 indexed citations
12.
Caplinger, M. A., et al.. (1999). An Archive of MGS/MOC Imaging Data. LPI. 1659.1 indexed citations
13.
Eliason, E. M., et al.. (1999). Clementine: A Multi-Spectral Digital Image Model Archive of the Moon. Lunar and Planetary Science Conference. 1812.16 indexed citations
14.
McEwen, A. S., E. M. Eliason, P. G. Lucey, et al.. (1998). Summary of Radiometric Calibration and Photometric Normalization Steps for the Clementine UVVIS Images. Lunar and Planetary Science Conference. 1466.46 indexed citations
15.
Becker, T. L., D. Cook, E. M. Eliason, et al.. (1997). Clementine UVVIS Multispectral Processing. LPI. 797.1 indexed citations
Kieffer, H. H., et al.. (1985). Intraband radiometric performance of the Landsat Thematic Mappers.. Photogrammetric Engineering & Remote Sensing. 51(9). 1331–1350.12 indexed citations
18.
Davis, Philip A., L. A. Soderblom, & E. M. Eliason. (1982). Rapid Extraction of Relative Topography from Viking Orbiter Imagery. Lunar and Planetary Science Conference. 144–145.
19.
Schaber, G. G., et al.. (1982). Venus Pioneer: Ratios and Composite Maps of Altimetry, RMS Slopes and the Fresnel Reflection Coefficient. Lunar and Planetary Science Conference. 683–684.
20.
Eliason, E. M. & L. A. Soderblom. (1977). An array processing system for lunar geochemical and geophysical data. Lunar and Planetary Science Conference Proceedings. 1. 1163–1170.15 indexed citations
Rankless uses publication and citation data sourced from OpenAlex, an open and comprehensive
bibliographic database. While OpenAlex provides broad and valuable coverage of the global
research landscape, it—like all bibliographic datasets—has inherent limitations. These include
incomplete records, variations in author disambiguation, differences in journal indexing, and
delays in data updates. As a result, some metrics and network relationships displayed in
Rankless may not fully capture the entirety of a scholar's output or impact.