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.
Emissivity of terrestrial materials in the 8–14 μm atmospheric window
1992622 citationsJohn W. Salisbury et al.profile →
Peers — A (Enhanced Table)
Peers by citation overlap · career bar shows stage (early→late)
cites ·
hero ref
Countries citing papers authored by John W. Salisbury
Since
Specialization
Citations
This map shows the geographic impact of John W. Salisbury'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 John W. Salisbury with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites John W. Salisbury more than expected).
Fields of papers citing papers by John W. Salisbury
This network shows the impact of papers produced by John W. Salisbury. 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 John W. Salisbury. The network helps show where John W. Salisbury may publish in the future.
Co-authorship network of co-authors of John W. Salisbury
This figure shows the co-authorship network connecting the top 25 collaborators of John W. Salisbury.
A scholar is included among the top collaborators of John W. Salisbury 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 John W. Salisbury. John W. Salisbury 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.
Kirkland, L. E., K. C. Herr, P. M. Adams, & John W. Salisbury. (2003). Hematite Coatings Match TES Spectra of Sinus Meridiani, Mars. Lunar and Planetary Science Conference. 1944.4 indexed citations
2.
Kirkland, L. E., K. C. Herr, P. M. Adams, Francès Westall, & John W. Salisbury. (2002). Spectra of Cemented, Hematite-rich Material and TES Spectra of Sinus Meridiani, Mars. LPI. 1218.3 indexed citations
3.
Kirkland, L. E., K. C. Herr, E. R. Keim, John W. Salisbury, & J. A. Hackwell. (2000). A Field Study of Thermal Infrared Spectra of Carbonates, with Implications for Studies of Mars. Lunar and Planetary Science Conference. 1876.4 indexed citations
4.
Kirkland, L. E., et al.. (1999). 1969 Mariner 7 Infrared Spectrometer: Data Recovery and Comparison to TES. Lunar and Planetary Science Conference. 1693.2 indexed citations
5.
Kirkland, L. E., et al.. (1999). 1969 Mariner Mars IRS Thermal Infrared Spectra of the Dark Side of Mars. LPI. 1687.
6.
Wald, Andrew & John W. Salisbury. (1992). Angular Dependence of Spectral Emissivity of Quartz and Basalt. LPI. 23. 1485.2 indexed citations
7.
Salisbury, John W., et al.. (1991). Mid-Infrared (2,08-14 microns) Spectra of Powdered Stony Meteorites. LPI. 22. 1161.1 indexed citations
8.
Nash, D. B. & John W. Salisbury. (1990). Infrared Reflectance Spectra of Plagioclase Feldspars. LPI. 21. 845.13 indexed citations
9.
Salisbury, John W., L. S. Walter, & Norma Vergo. (1989). Availability of a library of infrared (2.1-25.0 microns) mineral spectra. American Mineralogist. 74. 938–939.5 indexed citations
10.
Salisbury, John W., et al.. (1989). Measurement of Christiansen Frequencies in Spectra of Particulate Samples for Determination of Rock Composition. Lunar and Planetary Science Conference. 20. 940.6 indexed citations
11.
Salisbury, John W. & N. M. Milton. (1988). Thermal infrared (2.5- to 13.5-micrometer) directional hemispherical reflectance of leaves. Photogrammetric Engineering & Remote Sensing. 54(9). 1301–1304.53 indexed citations
12.
Walter, L. S., John W. Salisbury, & Norma Vergo. (1987). Spectral Variations in the Thermal Infrared Reststrahlen Band of Silicates. Lunar and Planetary Science Conference. 1052.1 indexed citations
13.
Podwysocki, M. H., John W. Salisbury, & Norma Vergo. (1985). Use of near-infrared spectra to distinguish between sedimentary cherts and hydrothermal silica associated with disseminated gold deposits. Geol. Soc. Am., Abstr. Programs; (United States). 17.4 indexed citations
Salisbury, John W., G. R. Hunt, & Lloyd M. Logan. (1973). Infrared spectra of Apollo 16 fines. 4. 3191.13 indexed citations
16.
Salisbury, John W., G. R. Hunt, & Lloyd M. Logan. (1973). Infrared Spectra of Apollo 16 Fines and Composition of Parent Material. LPI. 4. 647.1 indexed citations
17.
Salisbury, John W. & C. R. Chapman. (1973). Comparisons of Meteorite and Asteroid Spectral Reflectivities. Bulletin of the American Astronomical Society. 5. 308.1 indexed citations
18.
Logan, Lloyd M., et al.. (1972). Mid-Infrared Emission Spectrum of Apollo 14 Soil: Significance for Compositional Remote Sensing. Lunar and Planetary Science Conference. 3. 490.1 indexed citations
19.
Logan, Lloyd M., et al.. (1972). Midinfrared emission spectra of Apollo 14 and 15 soils and remote compositional mapping of the moon. Lunar and Planetary Science Conference Proceedings. 3. 3069.18 indexed citations
20.
Hunt, Graham R., John W. Salisbury, & Robert K. Vincent. (1968). Infrared Images of the Eclipsed Moon. S&T. 36. 223.2 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.