M. V. Alania

811 total citations
82 papers, 599 citations indexed

About

M. V. Alania is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Artificial Intelligence. According to data from OpenAlex, M. V. Alania has authored 82 papers receiving a total of 599 indexed citations (citations by other indexed papers that have themselves been cited), including 75 papers in Astronomy and Astrophysics, 24 papers in Nuclear and High Energy Physics and 22 papers in Artificial Intelligence. Recurrent topics in M. V. Alania's work include Solar and Space Plasma Dynamics (75 papers), Ionosphere and magnetosphere dynamics (52 papers) and Astrophysics and Cosmic Phenomena (22 papers). M. V. Alania is often cited by papers focused on Solar and Space Plasma Dynamics (75 papers), Ionosphere and magnetosphere dynamics (52 papers) and Astrophysics and Cosmic Phenomena (22 papers). M. V. Alania collaborates with scholars based in Poland, Georgia and Russia. M. V. Alania's co-authors include Anna Wawrzynczak, Agnieszka Gil, M. I. Tyasto, H. S. Ahluwalia, Л. И. Дорман, В. Е. Сдобнов, B. Szabelska, Shinsuke Abe and Tadeusz Wibig and has published in prestigious journals such as Solar Physics, Applied Mathematical Modelling and Advances in Space Research.

In The Last Decade

M. V. Alania

71 papers receiving 575 citations

Peers

M. V. Alania
Comparison fields: 5 of 30
  • Astronomy and Astrophysics 568
  • Artificial Intelligence 173
  • Atmospheric Science 154
  • Nuclear and High Energy Physics 138
  • Molecular Biology 38
Replace V. A. Oleneva with:
V. A. Oleneva Russia
М. А. Аbunina Russia
May‐Britt Kallenrode Germany
А. А. Аbunin Russia
L. I. Miroshnichenko Russia
O. P. M. Aslam South Africa
C. Lopate United States
Agnieszka Gil Poland
R. Gómez‐Herrero Germany
W. Dröge Germany
V. A. Oleneva Russia View profile →
Citations per field, relative to M. V. Alania
M. V. Alania · 1×
Citations per year, relative to M. V. Alania
M. V. Alania · 1×

Countries citing papers authored by M. V. Alania

Since Specialization
Citations

This map shows the geographic impact of M. V. Alania'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. V. Alania with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites M. V. Alania more than expected).

Fields of papers citing papers by M. V. Alania

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by M. V. Alania. 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. V. Alania. The network helps show where M. V. Alania may publish in the future.

Co-authorship network of co-authors of M. V. Alania

This figure shows the co-authorship network connecting the top 25 collaborators of M. V. Alania. A scholar is included among the top collaborators of M. V. Alania 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. V. Alania. M. V. Alania 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
# Work Indexed citations
1 4
2
3-D models of the Forbush decrease and 27-day variation of galactic cosmic rays with three dimensional divergence-free interplanetary magnetic field
1
3
ON THE NEW INDEX OF THE LONG-PERIOD MODULATION OF THE GALACTIC COSMIC RAYS INTENSITY
7
4
Mathematical Model of the Forbush Effect of the Galactic Cosmic Ray Intensity
0
5
Features of the Rigidity Spectrum of Galactic Cosmic Ray Intensity During the Recurrent Forbush Effect
2
6
27-Day Variations of the Galactic Cosmic Ray Intensity and Anisotropy
6
7
Fluctuations of the Interplanetary Magnetic Field During the Forbush Effects of Galactic Cosmic Rays
7
8
27-Day Variations Of The Galactic Cosmic Ray Intensity And Anisotropy In Different Solar Magnetic Cycles (1964-2004)
6
9
On the Relationship of the Interplanetary Magnetic Field Turbulence and the Energy Spectrum of the Forbush Effects
2
10
ON PECULIARITIES OF THE ANISOTROPIC DIFFUSION DURING FORBUSH EFFECTS OF GALACTIC COSMIC RAYS
1
11
ON THE RELATIONSHIP OF THE ENERGY SPEC- TRUM INDEXES OF THE 11-YEAR VARIATION OF GALACTIC COSMIC RAYS AND THE INTERPLAN- ETARY MAGNETIC FIELD STRENGTH FLUCTUA- TIONS
3
12
Modeling and Experimental Study of Short Period Changes in Galactic Cosmic Rays Intensity
1
13
Annual variation of galactic cosmic ray intensity and the role of the heliospheric current sheet
0
14
On the internal boundary condition's problem for the parker's transport equation of galactic cosmic rays
1
15
An Influence of Cosmic Rays and Geomagnetic Disturbances on the Cardiopathology Tendency
2
16
The Features of the 11-Year Modulation of Cosmic Rays and Large-Scale Fluctuations of Solar Wind
1
17
The Experimental and Theoretical Investigations of the of the Regular IMF Influence on the Spatial Distribution of Cosmic Ray Density and Anisotropy
2
18
Galactic Cosmic Ray Variations in the Heliosphere According to Radioactivity of Meteorites
0
19
The effect of the particle drift in cosmic ray anisotropy.
5
20
A new type of the quasiperiodic changes of cosmic ray anisotropy due to the particle drift in the sectors of the interplanetary magnetic field
2

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.

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