Citations per year, relative to R. Michard R. Michard (= 1×)
peers
G. D. Henson
Countries citing papers authored by R. Michard
Since
Specialization
Citations
This map shows the geographic impact of R. Michard'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. Michard with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites R. Michard more than expected).
This network shows the impact of papers produced by R. Michard. 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. Michard. The network helps show where R. Michard may publish in the future.
Co-authorship network of co-authors of R. Michard
This figure shows the co-authorship network connecting the top 25 collaborators of R. Michard.
A scholar is included among the top collaborators of R. Michard 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. Michard. R. Michard is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Michard, R., et al.. (1994). Quantitative morphology of E-S0 galaxies. III. Coded and parametric description of 108 galaxies in a complete sample. Astronomy & Astrophysics Supplement Series. 105(3). 481–501.4 indexed citations
8.
Michard, R., et al.. (1993). Quantitative morphology of E-S0 galaxies. I: Bulge, lens, disk and envelope in edge-on systems. Astronomy & Astrophysics Supplement Series. 98(1). 29–49.1 indexed citations
9.
Michard, R.. (1982). New UBV parameters for 46 E-SO galaxies in the Virgo cluster.. Astronomy & Astrophysics Supplement Series. 49. 591–606.1 indexed citations
10.
Michard, R.. (1980). On the M/L ratios in elliptical galaxies. A&A. 91. 122–128.1 indexed citations
Martres, M. J., et al.. (1966). Étude morphologique de la structure magnétique des régions actives en relation avec les phénomènes chromosphériques et les éruptions solaires. I. Classification magnétique et éruptivité. 29. 245.2 indexed citations
13.
Martres, M. J., et al.. (1966). Étude morphologique de la structure magnétique des régions actives en relation avec les phénomènes chromosphériques et les éruptions solaires. II. Localisation des plages brillantes, filaments et éruptions. 29. 249.4 indexed citations
14.
Michard, R., et al.. (1965). Observational studies of macroscopic inhomogeneities in the solar atmosphere. VII. A statistical analysis of photometric and kinematic inhomogeneities in the deep atmosphere. 28. 534.1 indexed citations
15.
Evans, J. W., et al.. (1963). Observational study of macroscopic inhomogeneities in the solar atmosphere. V. Statistical study of the time variations of the solar inhomogeneities. 26. 368.4 indexed citations
Michard, R., et al.. (1961). Champs magnétiques dans un centre d'activité solaire avant et pendant une éruption. 24. 54.2 indexed citations
18.
Michard, R.. (1954). Radial velocities of spicules and the width of chromospheric lines. Observatory. 74. 209–209.1 indexed citations
19.
Michard, R., et al.. (1954). Observations optiques et radioélectriques de l'éclipse totale de Soleil du 25 février 1952. 17. 317.1 indexed citations
20.
Michard, R.. (1953). Contribution à l'étude physique de la photosphère et des taches solaires. 16. 217.1 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.