Citations per year, relative to V. M. Malofeev V. M. Malofeev (= 1×)
peers
M. В. Попов
Countries citing papers authored by V. M. Malofeev
Since
Specialization
Citations
This map shows the geographic impact of V. M. Malofeev'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 V. M. Malofeev with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites V. M. Malofeev more than expected).
This network shows the impact of papers produced by V. M. Malofeev. 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 V. M. Malofeev. The network helps show where V. M. Malofeev may publish in the future.
Co-authorship network of co-authors of V. M. Malofeev
This figure shows the co-authorship network connecting the top 25 collaborators of V. M. Malofeev.
A scholar is included among the top collaborators of V. M. Malofeev 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 V. M. Malofeev. V. M. Malofeev is excluded from
the visualization to improve readability, since they are connected to all nodes in the network.
Malofeev, V. M., et al.. (2006). Pulsed Radio Emission From Two XDINS. 26. 31.
6.
Malofeev, V. M., et al.. (2006). Discovery of radio emission from X-ray pulsar XDINS 1RXS J214303.7 +065419+06. ATel. 798. 1.
7.
Malofeev, V. M., et al.. (1998). Discovery of a burst in one pulse component in the pulsar PSR B0643 + 80. 42(2). 241–245.1 indexed citations
8.
Shishov, V. I., et al.. (1995). Effect of turbulent interstellar plasma on the response of a radio interferometer.. Astronomy Reports. 39(4). 428–436.
9.
Seiradakis, J. H., D. A. Graham, A. Jessner, et al.. (1995). Pulsar profiles at high frequencies. I. The data.. 111. 205.1 indexed citations
10.
Малов, И. Ф., et al.. (1994). The observed integral radio luminosities of 232 pulsars.. AZh. 71. 762–767.
11.
Малов, И. Ф., et al.. (1994). Observed total radio luminosities of 232 pulsars. Astronomy Reports. 38(5). 677–682.2 indexed citations
12.
Malofeev, V. M.. (1993). Mean energy of weak pulsars at 102 and 61 MHz measurements.. Astronomy Letters. 19. 138.3 indexed citations
13.
Malofeev, V. M., et al.. (1989). Pulsar Mean Pulse Profiles at 102.5-MHZ. 33. 175.2 indexed citations
14.
Malofeev, V. M., et al.. (1989). The shapes of mean pulse profiles of pulsars'radio emission at the frequency 102,5 MHz.. Astronomicheskii Zhurnal. 66. 345–361.1 indexed citations
15.
Malofeev, V. M., et al.. (1988). Superdispersion Delay of Low-Frequency Pulsar Pulses. 14. 181.3 indexed citations
16.
Malofeev, V. M. & И. Ф. Малов. (1980). Mean spectra for 39 pulsars, and the interpretation of their characteristic features. 24. 54–63.1 indexed citations
Kuz’min, A. D., et al.. (1979). Radio flux density and pulse profile of pulsars at 102. 5 and 61 MHz. 23. 179.1 indexed citations
19.
Davies, Jon, et al.. (1978). Radio-emission spectra of five pulsars in the 17-1420 MHz range. 22. 1031–1039.1 indexed citations
20.
Малов, И. Ф., et al.. (1977). On the applicability of the hollow-cone beam model to pulsars.. 3. 442–445.
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.