К. Г. Иванов
About
In The Last Decade
К. Г. Иванов
67 papers receiving 248 citations
Peers
Comparison fields: 5 of 28
- Astronomy and Astrophysics 284
- Molecular Biology 135
- Geophysics 53
- Atmospheric Science 29
- Oceanography 16
Countries citing papers authored by К. Г. Иванов
This map shows the geographic impact of К. Г. Иванов'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 К. Г. Иванов with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites К. Г. Иванов more than expected).
Fields of papers citing papers by К. Г. Иванов
This network shows the impact of papers produced by К. Г. Иванов. 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 К. Г. Иванов. The network helps show where К. Г. Иванов may publish in the future.
Co-authorship network of co-authors of К. Г. Иванов
This figure shows the co-authorship network connecting the top 25 collaborators of К. Г. Иванов. A scholar is included among the top collaborators of К. Г. Иванов 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 К. Г. Иванов. К. Г. Иванов is excluded from the visualization to improve readability, since they are connected to all nodes in the network.
All Works
| # | Work | Indexed citations |
|---|---|---|
| 1 | Field draping around an interplanetary magnetic cloud with a shock wave | 0 |
| 2 | Filamentary solar wind. | 1 |
| 3 | Heliosphere-substorm 26 November - 5 December 1977. III. Geomagnetic deviations. | 3 |
| 4 | The interplanetary magnetic field as measured on "Phobos-2". Helio-geophysical conditions and sector structure. | 0 |
| 5 | Characteristics of the occurrence of Ps6 geomagnetic pulsations in connection with the interplanetary medium and the magnetopause | 1 |
| 6 | Interplanetary medium disturbances generated by a slow isolated magnetic cloud. | 1 |
| 7 | Shape of the magnetic cloud in the solar wind. | 1 |
| 8 | Specification of a phenomenological model of an interplanetary flare stream: a slow wave and boundary layer. | 1 |
| 9 | Classification of flare situations in connection with interplanetary and magnetospheric disturbances. | 1 |
| 10 | Geomagnetic storm and variations of galactic cosmic rays when passing a burst stream with complicated hydromagnetic structure. | 1 |
| 11 | Structure of Forbush decreases | 1 |
| 12 | Structure of typical nonstationary interplanetary plasma flow from direct-measurement data | 2 |
| 13 | Typical sequence of strong discontinuities in the head part of a non-stationary stream of the interplanetary plasma. | 2 |
| 14 | Front thickness of interplanetary shock waves | 1 |
| 15 | Deformation Velocity of the Solar Wind, Large-Scale Variations of the Interplanetary Magnetic Field, and the K p Index of Magnetic Activity | 1 |
| 16 | DID THE IMP 1 OBSERVE THE MAGNETIC WAKE OF THE MOON OR EARTH | 2 |
| 17 | The Height of the Explosion of the Tunguska Meteorite | 1 |
| 18 | Determination of the Earth's Conductivity from Data on DSt Variations | 1 |
| 19 | THE INFLUENCE OF A LOCAL INCREASE OF CONDUCTIVITY OF THE IONOSPHERE ON Sq VARIATION OF THE EARTH'S MAGNETIC FIELD | 2 |
| 20 | Morphological Regularities of Sudden Commencements of Magnetic Storms | 1 |
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.