D. Kiselman

2.7k total citations · 2 hit papers
46 papers, 1.9k citations indexed

About

D. Kiselman is a scholar working on Astronomy and Astrophysics, Atmospheric Science and Artificial Intelligence. According to data from OpenAlex, D. Kiselman has authored 46 papers receiving a total of 1.9k indexed citations (citations by other indexed papers that have themselves been cited), including 37 papers in Astronomy and Astrophysics, 11 papers in Atmospheric Science and 8 papers in Artificial Intelligence. Recurrent topics in D. Kiselman's work include Stellar, planetary, and galactic studies (30 papers), Solar and Space Plasma Dynamics (27 papers) and Astro and Planetary Science (16 papers). D. Kiselman is often cited by papers focused on Stellar, planetary, and galactic studies (30 papers), Solar and Space Plasma Dynamics (27 papers) and Astro and Planetary Science (16 papers). D. Kiselman collaborates with scholars based in Sweden, Australia and Germany. D. Kiselman's co-authors include M. Asplund, A. J. Sauval, N. Grevesse, C. Allende Prieto, Carlos Allende Prieto, G. B. Scharmer, M. G. Löfdahl, Tiago M. D. Pereira, L. Rouppe van der Voort and M. Carlsson and has published in prestigious journals such as Nature, Science and The Astrophysical Journal.

In The Last Decade

D. Kiselman

44 papers receiving 1.8k citations

Hit Papers

Line formation in solar granulation 2003 2026 2010 2018 2004 2003 100 200 300 400

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
D. Kiselman Sweden 19 1.8k 298 164 151 150 46 1.9k
Wolfgang Hayek Germany 21 1.8k 1.0× 402 1.3× 72 0.4× 88 0.6× 242 1.6× 26 1.9k
S. G. Korzennik United States 20 1.3k 0.7× 263 0.9× 82 0.5× 170 1.1× 55 0.4× 83 1.4k
T. Appourchaux France 24 1.6k 0.9× 484 1.6× 112 0.7× 103 0.7× 78 0.5× 125 1.7k
D. J. Christian United States 24 1.9k 1.1× 157 0.5× 78 0.5× 203 1.3× 49 0.3× 98 2.0k
M. Grewing Germany 13 1.4k 0.8× 71 0.2× 106 0.6× 122 0.8× 138 0.9× 87 1.5k
H. Holweger Germany 16 1.1k 0.6× 144 0.5× 42 0.3× 128 0.8× 140 0.9× 60 1.2k
J. G. Doyle United Kingdom 21 1.3k 0.7× 83 0.3× 54 0.3× 200 1.3× 66 0.4× 111 1.4k
Steven H. Saar United States 32 3.2k 1.8× 768 2.6× 63 0.4× 109 0.7× 58 0.4× 108 3.2k
Sven Wedemeyer Norway 22 1.6k 0.9× 132 0.4× 231 1.4× 65 0.4× 164 1.1× 81 1.7k
Christopher M. Johns‐Krull United States 38 3.9k 2.2× 386 1.3× 86 0.5× 113 0.7× 162 1.1× 100 4.0k

Countries citing papers authored by D. Kiselman

Since Specialization
Citations

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

Fields of papers citing papers by D. Kiselman

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of D. Kiselman

This figure shows the co-authorship network connecting the top 25 collaborators of D. Kiselman. A scholar is included among the top collaborators of D. Kiselman 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 D. Kiselman. D. Kiselman 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.
Lind, K., et al.. (2023). 3D non-LTE modeling of the stellar center-to-limb variation for transmission spectroscopy studies. Astronomy and Astrophysics. 683. A242–A242. 5 indexed citations
2.
Solanki, S. K., et al.. (2022). A prototype of a microlensed hyperspectral imager for solar observations. Astronomy and Astrophysics. 668. A149–A149. 17 indexed citations
3.
Kiselman, D., et al.. (2022). Center-to-limb variation of spectral lines and continua observed with SST/CRISP and SST/CHROMIS. Astronomy and Astrophysics. 671. A130–A130. 16 indexed citations
4.
Henriques, V. M. J., E. Scullion, M. Mathioudakis, et al.. (2015). Stable umbral chromospheric structures. Springer Link (Chiba Institute of Technology). 6 indexed citations
5.
Henriques, V. M. J. & D. Kiselman. (2013). Ca II H sunspot tomography from the photosphere to the chromosphere. Astronomy and Astrophysics. 557. A5–A5. 6 indexed citations
6.
Kiselman, D., Tiago M. D. Pereira, B. Gustafsson, et al.. (2011). Is the solar spectrum latitude-dependent?. Astronomy and Astrophysics. 535. A14–A14. 38 indexed citations
7.
Rodríguez, J. de la Cruz, D. Kiselman, & M. Carlsson. (2011). Solar velocity references from 3D HD photospheric models. Astronomy and Astrophysics. 528. A113–A113. 32 indexed citations
8.
Löfdahl, M. G., V. M. J. Henriques, & D. Kiselman. (2011). A tilted interference filter in a converging beam. Astronomy and Astrophysics. 533. A82–A82. 17 indexed citations
9.
Fabbian, D., M. Asplund, P. S. Barklem, M. Carlsson, & D. Kiselman. (2009). Neutral oxygen spectral line formation revisitedwith new collisional data: large departuresfrom LTE at low metallicity. Springer Link (Chiba Institute of Technology). 46 indexed citations
10.
Henriques, V. M. J. & D. Kiselman. (2009). Temperature stratification in the Sun's photosphere in high horizontal resolution using Ca II H filtergrams.. Memorie della Societa Astronomica Italiana. 80. 639.
11.
Pereira, Tiago M. D., D. Kiselman, & M. Asplund. (2009). Oxygen lines in solar granulation. Astronomy and Astrophysics. 507(1). 417–432. 33 indexed citations
12.
Scharmer, G. B., V. M. J. Henriques, D. Kiselman, et al.. (2008). Spectropolarimetry of Sunspots at 0.16 ARCSEC resolution. 12. 2 indexed citations
13.
Langhans, K., G. B. Scharmer, D. Kiselman, & M. G. Löfdahl. (2007). Observations of dark-cored filaments in sunspot penumbrae. Astronomy and Astrophysics. 464(2). 763–774. 33 indexed citations
14.
Fabbian, D., M. Asplund, M. Carlsson, & D. Kiselman. (2006). The non-LTE line formation of neutral carbon in late-type stars. Astronomy and Astrophysics. 458(3). 899–914. 33 indexed citations
15.
Langhans, K., G. B. Scharmer, D. Kiselman, M. G. Löfdahl, & Thomas Berger. (2005). Inclination of magnetic fields and flows in sunspot penumbrae. Astronomy and Astrophysics. 436(3). 1087–1101. 72 indexed citations
16.
Voort, L. Rouppe van der, M. G. Löfdahl, D. Kiselman, & G. B. Scharmer. (2004). Penumbral structure at 0$\farcs$1 resolution. Astronomy and Astrophysics. 414(2). 717–726. 48 indexed citations
17.
Asplund, M., N. Grevesse, A. J. Sauval, C. Allende Prieto, & D. Kiselman. (2004). Line formation in solar granulation. Astronomy and Astrophysics. 417(2). 751–768. 467 indexed citations breakdown →
18.
Scharmer, G. B., B. V. Gudiksen, D. Kiselman, M. G. Löfdahl, & L. Rouppe van der Voort. (2002). Dark cores in sunspot penumbral filaments. Nature. 420(6912). 151–153. 144 indexed citations
19.
Kiselman, D. & M. Asplund. (2001). Spatially Resolved Solar Lines as Diagnostics of NLTE Effects (CD-ROM Directory: contribs/kiselman). ASPC. 223. 684. 1 indexed citations
20.
Kiselman, D.. (1994). High-spatial-resolution solar observations of spectral lines used for abundance analysis. Astronomy & Astrophysics Supplement Series. 104(1). 23–77. 4 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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