This map shows the geographic impact of M. Leitner'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 M. Leitner with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites M. Leitner more than expected).
This network shows the impact of papers produced by M. Leitner. 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 M. Leitner. The network helps show where M. Leitner may publish in the future.
Co-authorship network of co-authors of M. Leitner
This figure shows the co-authorship network connecting the top 25 collaborators of M. Leitner.
A scholar is included among the top collaborators of M. Leitner 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 M. Leitner. M. Leitner 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.
Vršnak, B., Tanja Amerstorfer, Mateja Dumbović, et al.. (2019). Heliospheric Evolution of Magnetic Clouds. The Astrophysical Journal. 877(2). 77–77.26 indexed citations
2.
Yu, Wenyuan, C. J. Farrugia, Noé Lugaz, et al.. (2013). https://dx.doi.org/10.1002/2013ja019115A Statistical Analysis of Properties of Small Transients in the Solar Wind 2007-2009: STEREO and Wind Observations. University of New Hampshire Scholars Repository (University of New Hampshire at Manchester). 2013. 154.30 indexed citations
3.
Farrugia, C. J., D. B. Berdichevsky, A. B. Galvin, et al.. (2010). Multiple, Distant (40 deg) in situ Observations of a Magnetic Cloud and a Corotating Interaction Region Complex. AGU Fall Meeting Abstracts. 2010.2 indexed citations
Leitner, M., C. J. Farrugia, M. Maksimović, et al.. (2010). Solar wind quasi invariant within ICMEs. AIP conference proceedings. 652–654.2 indexed citations
Möstl, Christian, C. J. Farrugia, C. Miklenic, et al.. (2008). https://dx.doi.org/10.1029/2008ja013657Multi-spacecraft Recovery of a Magnetic Cloud and its Origin From Magnetic Reconnection on the Sun. University of New Hampshire Scholars Repository (University of New Hampshire at Manchester). 2008.3 indexed citations
Leitner, M., C. J. Farrugia, V. A. Osherovich, et al.. (2005). The relative distribution of the magnetic and plasma kinetic energy densities in the inner heliosphere (< 1 AU). ESASP. 592. 743.6 indexed citations
Leitner, M., C. J. Farrugia, H. K. Biernat, et al.. (2005). On the thickness of the sheath of magnetic clouds in the inner heliosphere: a Helios - Wind investigation. Max Planck Institute for Plasma Physics. 592. 739–742.2 indexed citations
15.
Rucker, H. O., G. V. Litvinenko, Ulrich Taubenschuss, et al.. (2004). Superfine Structure of Jovian Millisecond Radio Bursts. AGUSM. 2004.1 indexed citations
Leitner, M. & H. O. Rucker. (2003). A Digital Broadband Waveform Receiving System for Fast Radio Emissions in the Decametric Range. EAEJA. 1576.1 indexed citations
18.
Biernat, H. K., C. J. Farrugia, M. Leitner, et al.. (2003). Evolution of interplanetary magnetic clouds from 0.3 AU to 1 AU: A joint Helios-Wind Study. AGU Fall Meeting Abstracts. 2003.1 indexed citations
Leitner, M. & H. O. Rucker. (2001). Waveform Analysis Techniques of Jovian S-Burst Observations. 91–95.2 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.