V. M. Malofeev
About
In The Last Decade
V. M. Malofeev
56 papers receiving 448 citations
Peers
Comparison fields: 5 of 29
- Astronomy and Astrophysics 429
- Nuclear and High Energy Physics 199
- Ocean Engineering 60
- Oceanography 58
- Geophysics 58
Countries citing papers authored by V. M. Malofeev
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).
Fields of papers citing papers by V. M. Malofeev
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.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | 1 | |
| 2 | 1 | |
| 3 | 20 | |
| 4 | 0 | |
| 5 | Pulsed Radio Emission From Two XDINS | 0 |
| 6 | Discovery of radio emission from X-ray pulsar XDINS 1RXS J214303.7 +065419+06 | 0 |
| 7 | Discovery of a burst in one pulse component in the pulsar PSR B0643 + 80 | 1 |
| 8 | Effect of turbulent interstellar plasma on the response of a radio interferometer. | 0 |
| 9 | Pulsar profiles at high frequencies. I. The data. | 1 |
| 10 | The observed integral radio luminosities of 232 pulsars. | 0 |
| 11 | Observed total radio luminosities of 232 pulsars | 2 |
| 12 | Mean energy of weak pulsars at 102 and 61 MHz measurements. | 3 |
| 13 | Pulsar Mean Pulse Profiles at 102.5-MHZ | 2 |
| 14 | The shapes of mean pulse profiles of pulsars'radio emission at the frequency 102,5 MHz. | 1 |
| 15 | Superdispersion Delay of Low-Frequency Pulsar Pulses | 3 |
| 16 | Mean spectra for 39 pulsars, and the interpretation of their characteristic features | 1 |
| 17 | 7 | |
| 18 | Radio flux density and pulse profile of pulsars at 102. 5 and 61 MHz | 1 |
| 19 | Radio-emission spectra of five pulsars in the 17-1420 MHz range | 1 |
| 20 | On the applicability of the hollow-cone beam model to pulsars. | 0 |
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.