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.
Plasma Crystal: Coulomb Crystallization in a Dusty Plasma
19941.3k citationsHubertus M. Thomas, G. E. Morfill et al.Physical Review Lettersprofile →
Plasma medicine: an introductory review
20091.3k citationsG. E. Morfill, Tetsuji Shimizu et al.profile →
A first prospective randomized controlled trial to decrease bacterial load using cold atmospheric argon plasma on chronic wounds in patients
2010568 citationsGeorg Isbary, G. E. Morfill 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 G. E. Morfill'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 G. E. Morfill with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites G. E. Morfill more than expected).
This network shows the impact of papers produced by G. E. Morfill. 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 G. E. Morfill. The network helps show where G. E. Morfill may publish in the future.
Co-authorship network of co-authors of G. E. Morfill
This figure shows the co-authorship network connecting the top 25 collaborators of G. E. Morfill.
A scholar is included among the top collaborators of G. E. Morfill 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 G. E. Morfill. G. E. Morfill is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Klumov, B. A., G. E. Morfill, & S. I. Popel. (2005). Formation of structures in a dusty ionosphere. Journal of Experimental and Theoretical Physics. 100(1). 152–164.81 indexed citations
Goree, J., G. E. Morfill, & В. Н. Цытович. (1998). Excitation of collective plasma modes during collisions between dust grains and the formation of dust plasma crystals. Plasma Physics Reports. 24(6). 490–497.1 indexed citations
10.
Tsytovich, V. N., et al.. (1998). Radiative dust cooling and dust agglomeration in plasmas. Max Planck Institute for Plasma Physics. 18(5). 281–291.16 indexed citations
11.
Staubach, P., S. F. Dermott, H. Fechtig, et al.. (1997). South-north and radial traverses through the zodiacal cloud. Lund University Publications (Lund University).2 indexed citations
12.
Grüen, E., H. Fechtig, J. Kissel, et al.. (1992). The Ulysses dust experiment. OpenGrey (Institut de l'Information Scientifique et Technique). 92(2). 411–423.86 indexed citations
13.
Mann, Ingrid, E. Grün, M. Baguhl, et al.. (1992). Measurements with the Ulysses and Galileo dust detectors close to the ecliptic. 30. 13.1 indexed citations
14.
Grün, E., M. Baguhl, H. Fechtig, et al.. (1991). Interplanetary Dust Near 1 AU. 765. 76.2 indexed citations
15.
Grün, E., M. Baguhl, H. Fechtig, et al.. (1991). Interplanetary Dust Observed by Galileo and Ulysses. Bulletin of the American Astronomical Society. 23. 1149.2 indexed citations
16.
Morfill, G. E., W. M. Tscharnuter, & H. J. Voêlk. (1985). Dynamical and chemical evolution of the protoplanetary nebula.. 493–533.29 indexed citations
17.
Morfill, G. E. & L. O’C. Drury. (1981). a Constraint on Prompt Supernova Cosmic-Ray Production from Gamma-Ray Observations. International Cosmic Ray Conference. 1. 172.
18.
Morfill, G. E., E. Grüen, & T. V. Johnson. (1980). Dust in Jupiter's magnetosphere. I - Physical processes. II - Origin of the ring. III - Time variations. IV - Effect on magnetospheric electrons and ions. Planetary and Space Science. 28.2 indexed citations
19.
Forman, M. A. & G. E. Morfill. (1979). Time-Dependent Acceleration of Solar Wind Plasma to Mev Energies at Corotating Interplanetary Shocks. ICRC. 5. 328.3 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.