This map shows the geographic impact of J. Engelmann'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 J. Engelmann with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites J. Engelmann more than expected).
This network shows the impact of papers produced by J. Engelmann. 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 J. Engelmann. The network helps show where J. Engelmann may publish in the future.
Co-authorship network of co-authors of J. Engelmann
This figure shows the co-authorship network connecting the top 25 collaborators of J. Engelmann.
A scholar is included among the top collaborators of J. Engelmann 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 J. Engelmann. J. Engelmann is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Koch, Frieder, et al.. (2015). Through pitch monitoring by optical scatterometry. Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE. 9424. 942429–942429.1 indexed citations
Engelmann, J., P. Ferrando, A. Soutoul, et al.. (1990). Charge composition and energy spectra of cosmic-ray nuclei for elements from Be to Ni - Results from HEAO-3-C2.. 233(1). 96–111.153 indexed citations
Soutoul, A., J. Engelmann, P. Ferrando, et al.. (1985). Charge and energy dependence of the residence time of cosmic ray nuclei below 15 GeV/nucleon. NASA Technical Reports Server (NASA). 2. 8.2 indexed citations
9.
Engelmann, J., P. Goret, E. Juliusson, et al.. (1985). Source energy spectra of heavy cosmic ray nuclei as derived from the French-Danish experiment on HEAO-3. 148(1). 12–20.12 indexed citations
10.
Juliusson, E., J. Engelmann, L. Koch-Miramond, et al.. (1983). The Galactic Cosmic Ray Energy Spectra as Measured by the French-Danish Instrument on HEAD-3. ICRC. 2. 21.4 indexed citations
11.
Koch-Miramond, L., J. Engelmann, P. Goret, et al.. (1983). Energy spectra of cosmic rays at source as derived from the French-Danish experiment on HEAO-3.. International Cosmic Ray Conference. 2. 219.1 indexed citations
Soutoul, A., J. Engelmann, P. Goret, et al.. (1981). Isotope Analysis Using the Geomagnetic Method. International Cosmic Ray Conference. 9. 105–108.2 indexed citations
14.
Engelmann, J., P. Goret, E. Juliusson, et al.. (1981). The elemental composition of cosmic rays from Be to Zn as measured by the French Danish instrument on HEAO-3. ICRC. 2. 17.8 indexed citations
15.
Perron, C., J. Engelmann, P. Goret, et al.. (1981). Interpretation of the elemental abundances measured by the French-Danish experiment on HEAO-3 - Interstellar propagation and derivation of source abundances. ICRC. 9. 118–121.2 indexed citations
Barouch, Eytan, et al.. (1969). Simultaneous satellite and rocket observations of the February 25th 1969 solar proton event. Acta physica Hungarica. 2. 493–499.2 indexed citations
20.
Engelmann, J., et al.. (1969). ENERGY SPECTRA AND TIME PROFILE OF PROTONS EMITTED DURING THE SOLAR FLARE OF JUNE 9, 1968.. International Cosmic Ray Conference. 2. 487–491.2 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.