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.
Global Distribution of Crustal Magnetization Discovered by the Mars Global Surveyor MAG/ER Experiment
1999792 citationsM. H. Acuña, R. P. Lin et al.profile →
A three-dimensional plasma and energetic particle investigation for the wind spacecraft
1995642 citationsR. P. Lin, K. A. Anderson et al.profile →
Magnetic Field and Plasma Observations at Mars: Initial Results of the Mars Global Surveyor Mission
1998576 citationsM. H. Acuña, R. P. Lin et al.profile →
The MAVEN Solar Wind Electron Analyzer
2016250 citationsD. L. Mitchell, D. W. Curtis et al.profile →
Author Peers
Peers are selected by citation overlap in the author's most active subfields.
citations ·
hero ref
This map shows the geographic impact of R. P. Lin'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 R. P. Lin with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites R. P. Lin more than expected).
This network shows the impact of papers produced by R. P. Lin. 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 R. P. Lin. The network helps show where R. P. Lin may publish in the future.
Co-authorship network of co-authors of R. P. Lin
This figure shows the co-authorship network connecting the top 25 collaborators of R. P. Lin.
A scholar is included among the top collaborators of R. P. Lin 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 R. P. Lin. R. P. Lin 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.
Howard, R. A., A. Vourlidas, D. A. Biesecker, et al.. (2012). A Space Weather Mission to the Earth's 5th Lagrangian Point (L5). AGU Fall Meeting Abstracts. 2012.1 indexed citations
2.
Lillis, R. J., et al.. (2007). Magnetic Signatures and Crater Retention Ages of Giant Buried Basins on Mars: New Constraints on the Timing of the Ancient Dynamo. 1353. 3090.1 indexed citations
3.
Fivian, M. D., H. S. Hudson, R. P. Lin, & H. Jabran Zahid. (2007). Solar Shape Measurements from RHESSI: A Large Excess Oblateness. AGU Fall Meeting Abstracts. 2007.6 indexed citations
4.
Krucker, S., G. J. Hurford, & R. P. Lin. (2005). RHESSI X-ray and Gamma-ray observations of the January 20, 2005 event. AGU Fall Meeting Abstracts. 2005.3 indexed citations
5.
Lin, R. P., et al.. (2005). Comparison between impulsive 3He-rich events and energetic electron events. AGUSM. 2005.1 indexed citations
6.
Shih, Albert Y., et al.. (2004). RHESSI Spectroscopy of Nuclear De-excitation Lines in X-class Flares. cosp. 204. 4135.2 indexed citations
7.
Gopalswamy, N., et al.. (2003). Why was there no Solar Energetic Particle Event Associated with the Gamma-ray-line Flare of 2002 July 23?.1 indexed citations
8.
Øieroset, M., R. P. Lin, T. D. Phan, D. E. Larson, & S. D. Bale. (2002). Evidence for Electron Acceleration up to ~300 keV in the Magnetic Reconnection Diffusion Region of the Earth's Magnetotail. AGUFM. 2002.6 indexed citations
9.
Frey, S., J. S. Halekas, D. L. Mitchell, & R. P. Lin. (2002). CLUSTER ANALYSIS OF LUNAR MAGNETISM, GRAVITY ANOMALIES, AND TOPOLOGY.S. Frey,. Lunar and Planetary Science Conference. 2048.1 indexed citations
10.
Sibeck, D. G., T. D. Phan, R. P. Lin, & R. P. Lepping. (2002). Wind Observations of Foreshock Cavities. AGUSM. 2002.2 indexed citations
11.
Salem, C. S., C. Lacombe, A. Mangeney, et al.. (2001). ELECTRON PROPERTIES AND COULOMB COLLISIONS IN THE SOLAR WIND AT 1 AU: WIND OBSERVATIONS. AGU Fall Meeting Abstracts. 2001.2 indexed citations
12.
Lin, R. P., et al.. (2001). The High Energy Solar Spectroscopic Imager (HESSI) Small Explorer mission for the next (2000) solar maximum. ICRC. 27. 209.2 indexed citations
13.
Halekas, J. S., D. L. Mitchell, R. P. Lin, et al.. (2000). Mapping of the Lunar Crustal Magnetic Field by Lunar Prospector. Lunar and Planetary Science Conference. 1436.2 indexed citations
14.
Lin, R. P., et al.. (1999). Initial Maps of the Crustal Magnetic Field of the Moon Using Lunar Prospector Magnetometer Data. Lunar and Planetary Science Conference. 1382.1 indexed citations
15.
Lin, R. P., et al.. (1999). Initial Measurements of the Lunar Induced Magnetic Moment in the Geomagnetic Tail Using Lunar Prospector Data. Lunar and Planetary Science Conference. 1402.1 indexed citations
16.
d’Uston, C., H. Rème, J. A. Sauvaud, et al.. (1986). Description of the main boundaries seen by the Giotto electron experiment inside the Comet Halley-solar wind interaction regions. 250. 77–80.1 indexed citations
17.
Anderson, K. A., C. W. Carlson, D. W. Curtis, et al.. (1986). The upstream region, foreshock and bow shock wave at Halley's Comet from plasma electron measurements. 250. 259–261.2 indexed citations
18.
Anderson, K. A., R. P. Lin, J. E. McCoy, et al.. (1976). The Large Magnetized Region Associated with Rima Sirsalis. Lunar and Planetary Science Conference. 7. 16.2 indexed citations
19.
Álvarez, H. & R. P. Lin. (1975). Interplanetary Scattering of Fast Solar Electrons Deduced from Type-III Burst Observed at Km-Wavelength. Bulletin of the American Astronomical Society. 7. 366.5 indexed citations
20.
Lin, R. P. & K. A. Anderson. (1973). Energetic Solar Electrons Accompanying Type III Bursts Observed at 1 A. U.. Bulletin of the American Astronomical Society. 5. 275.1 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.