M. Selwa

508 total citations
20 papers, 400 citations indexed

About

M. Selwa is a scholar working on Astronomy and Astrophysics, Molecular Biology and Nuclear and High Energy Physics. According to data from OpenAlex, M. Selwa has authored 20 papers receiving a total of 400 indexed citations (citations by other indexed papers that have themselves been cited), including 19 papers in Astronomy and Astrophysics, 7 papers in Molecular Biology and 4 papers in Nuclear and High Energy Physics. Recurrent topics in M. Selwa's work include Ionosphere and magnetosphere dynamics (19 papers), Solar and Space Plasma Dynamics (19 papers) and Geomagnetism and Paleomagnetism Studies (7 papers). M. Selwa is often cited by papers focused on Ionosphere and magnetosphere dynamics (19 papers), Solar and Space Plasma Dynamics (19 papers) and Geomagnetism and Paleomagnetism Studies (7 papers). M. Selwa collaborates with scholars based in United States, Poland and Germany. M. Selwa's co-authors include K. Murawski, S. K. Solanki, L. Ofman, Tongjiang Wang, C. R. DeVore, Stefaan Poedts, G. Tóth, G. Kowal, U. Shumlak and Marcin Gruszecki and has published in prestigious journals such as The Astrophysical Journal, Astronomy and Astrophysics and Solar Physics.

In The Last Decade

M. Selwa

20 papers receiving 398 citations

Peers — A (Enhanced Table)

Peers by citation overlap · career bar shows stage (early→late) cites · hero ref

Name h Career Trend Papers Cites
M. Selwa United States 14 399 189 33 17 4 20 400
C. H. An United States 9 259 0.6× 103 0.5× 34 1.0× 10 0.6× 2 0.5× 24 267
Sergey Lesovoi Russia 10 285 0.7× 101 0.5× 40 1.2× 33 1.9× 10 2.5× 35 292
Vyacheslav S. Titov Germany 5 329 0.8× 107 0.6× 45 1.4× 4 0.2× 10 2.5× 5 337
M. Ohyama Japan 9 334 0.8× 78 0.4× 35 1.1× 9 0.5× 14 3.5× 14 339
W. P. Guo United States 9 445 1.1× 155 0.8× 10 0.3× 14 0.8× 7 1.8× 15 446
А. Н. Коржавин Russia 8 292 0.7× 77 0.4× 29 0.9× 64 3.8× 14 3.5× 43 298
A. H. Wang United States 9 332 0.8× 73 0.4× 12 0.4× 16 0.9× 10 2.5× 12 338
E. Romashets Czechia 11 379 0.9× 212 1.1× 19 0.6× 9 0.5× 15 3.8× 63 398
B. von Rekowski United Kingdom 9 220 0.6× 44 0.2× 22 0.7× 6 0.4× 5 1.3× 16 224

Countries citing papers authored by M. Selwa

Since Specialization
Citations

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

Fields of papers citing papers by M. Selwa

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of M. Selwa

This figure shows the co-authorship network connecting the top 25 collaborators of M. Selwa. A scholar is included among the top collaborators of M. Selwa 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. Selwa. M. Selwa 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.
Selwa, M., Stefaan Poedts, & C. R. DeVore. (2013). Numerical Simulations of Dome-Shaped EUV Waves from Different Active-Region Configurations. Solar Physics. 284(2). 515–539. 6 indexed citations
2.
Selwa, M., Stefaan Poedts, & C. R. DeVore. (2012). DOME-SHAPED EUV WAVES FROM ROTATING ACTIVE REGIONS. The Astrophysical Journal Letters. 747(2). L21–L21. 18 indexed citations
3.
Selwa, M., S. K. Solanki, & L. Ofman. (2011). THE ROLE OF ACTIVE REGION LOOP GEOMETRY. II. SYMMETRY BREAKING IN THREE-DIMENSIONAL ACTIVE REGION: WHY ARE VERTICAL KINK OSCILLATIONS OBSERVED SO RARELY?. The Astrophysical Journal. 728(2). 87–87. 15 indexed citations
4.
Selwa, M., L. Ofman, & S. K. Solanki. (2010). THE ROLE OF ACTIVE REGION LOOP GEOMETRY. I. HOW CAN IT AFFECT CORONAL SEISMOLOGY?. The Astrophysical Journal. 726(1). 42–42. 14 indexed citations
5.
Selwa, M. & L. Ofman. (2010). THE ROLE OF ACTIVE REGION TOPOLOGY IN EXCITATION, TRAPPING, AND DAMPING OF CORONAL LOOP OSCILLATIONS. The Astrophysical Journal. 714(1). 170–177. 14 indexed citations
6.
Selwa, M., K. Murawski, S. K. Solanki, & L. Ofman. (2009). Excitation of vertical kink waves in a solar coronal arcade loop by a periodic driver. Astronomy and Astrophysics. 512. A76–A76. 10 indexed citations
7.
Selwa, M. & L. Ofman. (2009). 3-D numerical simulations of coronal loops oscillations. Annales Geophysicae. 27(10). 3899–3908. 21 indexed citations
8.
Wang, Tongjiang, S. K. Solanki, & M. Selwa. (2008). Identification of different types of kink modes in coronal loops: principles and application to TRACE results. Springer Link (Chiba Institute of Technology). 22 indexed citations
9.
Ofman, L. & M. Selwa. (2008). Three-dimensional MHD modeling of waves in active region loops. Proceedings of the International Astronomical Union. 4(S257). 151–154. 2 indexed citations
10.
Selwa, M., L. Ofman, & K. Murawski. (2007). Numerical Simulations of Slow Standing Waves in a Curved Solar Coronal Loop. The Astrophysical Journal. 668(1). L83–L86. 39 indexed citations
11.
Gruszecki, Marcin, K. Murawski, M. Selwa, & L. Ofman. (2006). Numerical simulations of vertical oscillations of a multi-stranded coronal loop. Astronomy and Astrophysics. 460(3). 887–892. 21 indexed citations
12.
Selwa, M., K. Murawski, S. K. Solanki, & Tongjiang Wang. (2006). Energy leakage as an attenuation mechanism for vertical kink oscillations in solar coronalwave guides. Astronomy and Astrophysics. 462(3). 1127–1135. 31 indexed citations
13.
Selwa, M., et al.. (2006). Numerical simulations of impulsively generated vertical oscillations in a solar coronal arcade loop. Astronomy and Astrophysics. 454(2). 653–661. 30 indexed citations
14.
Murawski, K., M. Selwa, & Luigi Nocera. (2005). Numerical simulations of fast magnetosonic waves in a curved coronal loop. Astronomy and Astrophysics. 437(2). 687–690. 13 indexed citations
15.
Selwa, M., K. Murawski, & S. K. Solanki. (2005). Excitation and damping of slow magnetosonic standing waves in a solar coronal loop. Astronomy and Astrophysics. 436(2). 701–709. 65 indexed citations
16.
Selwa, M., et al.. (2005). Numerical simulations of vertical oscillations of a solar coronal loop. Astronomy and Astrophysics. 440(1). 385–390. 36 indexed citations
17.
Murawski, K., M. Selwa, & James A. Rossmanith. (2005). Numerical Simulations of Vertical Oscillations of a Curved Coronal Loop. Solar Physics. 231(1-2). 87–94. 12 indexed citations
18.
Selwa, M., K. Murawski, & G. Kowal. (2004). Three-dimensional numerical simulations of impulsively generated MHD waves in solar coronal loops. Astronomy and Astrophysics. 422(3). 1067–1072. 18 indexed citations
19.
Selwa, M., R. Skartlien, & K. Murawski. (2004). Numerical simulations of stochastically excited sound waves in arandom medium. Astronomy and Astrophysics. 420(3). 1123–1127. 3 indexed citations
20.
Selwa, M. & K. Murawski. (2004). Numerical simulations of impulsively generated mass density perturbations in a solar coronal loop. Astronomy and Astrophysics. 425(2). 719–724. 10 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.

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