K. Langhans

410 total citations
10 papers, 268 citations indexed

About

K. Langhans is a scholar working on Astronomy and Astrophysics, Artificial Intelligence and Molecular Biology. According to data from OpenAlex, K. Langhans has authored 10 papers receiving a total of 268 indexed citations (citations by other indexed papers that have themselves been cited), including 10 papers in Astronomy and Astrophysics, 3 papers in Artificial Intelligence and 1 paper in Molecular Biology. Recurrent topics in K. Langhans's work include Solar and Space Plasma Dynamics (9 papers), Stellar, planetary, and galactic studies (7 papers) and Solar Radiation and Photovoltaics (3 papers). K. Langhans is often cited by papers focused on Solar and Space Plasma Dynamics (9 papers), Stellar, planetary, and galactic studies (7 papers) and Solar Radiation and Photovoltaics (3 papers). K. Langhans collaborates with scholars based in Germany, Sweden and Netherlands. K. Langhans's co-authors include D. Kiselman, W. Schmidt, G. B. Scharmer, M. G. Löfdahl, A. Tritschler, Thomas Berger, R. Schlichenmaier, L. R. Bellot Rubio, T. Kentischer and M. Asplund and has published in prestigious journals such as The Astrophysical Journal, Astronomy and Astrophysics and Solar Physics.

In The Last Decade

K. Langhans

10 papers receiving 261 citations

Peers — A (Enhanced Table)

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

Name	h						Papers	Cites
K. Langhans Germany	8	262	74	39	38	20	10	268
M. Heiko Franz Germany	7	275 1.0×	65 0.9×	44 1.1×	49 1.3×	14 0.7×	13	306
J. E. Simmons United States	6	240 0.9×	47 0.6×	28 0.7×	51 1.3×	15 0.8×	10	290
Isabelle Scholl United States	10	296 1.1×	55 0.7×	19 0.5×	62 1.6×	14 0.7×	24	312
C. Westendorp Plaza Spain	5	298 1.1×	109 1.5×	23 0.6×	45 1.2×	27 1.4×	10	301
M. Verma Germany	12	299 1.1×	87 1.2×	15 0.4×	46 1.2×	27 1.4×	41	312
A. Pietarila United States	13	444 1.7×	65 0.9×	32 0.8×	78 2.1×	17 0.8×	21	449
R. Falciani Italy	10	381 1.5×	50 0.7×	19 0.5×	60 1.6×	25 1.3×	42	395
R. Shine United States	5	399 1.5×	59 0.8×	23 0.6×	116 3.1×	11 0.6×	8	410
A. V. Panasyuk United States	10	393 1.5×	25 0.3×	20 0.5×	45 1.2×	7 0.3×	24	403
Dali Georgobiani United States	10	274 1.0×	35 0.5×	19 0.5×	43 1.1×	10 0.5×	23	301

Countries citing papers authored by K. Langhans

Since Specialization

Citations

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

Fields of papers citing papers by K. Langhans

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of K. Langhans

This figure shows the co-authorship network connecting the top 25 collaborators of K. Langhans. A scholar is included among the top collaborators of K. Langhans 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 K. Langhans. K. Langhans is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

Sort: Min cites: Since: Top N: Style:

10 of 10 papers shown

1.

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

2.

Rubio, L. R. Bellot, R. Schlichenmaier, & K. Langhans. (2010). SEARCHING FOR OVERTURNING CONVECTION IN PENUMBRAL FILAMENTS: SLIT SPECTROSCOPY AT 0.″2 RESOLUTION. The Astrophysical Journal. 725(1). 11–16. 9 indexed citations

3.

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

4.

Scharmer, G. B., K. Langhans, D. Kiselman, & M. G. Löfdahl. (2007). Recent High Resolution Observations and Interpretations of Sunspot Fine Structure. 369. 71. 2 indexed citations

5.

Rubio, L. R. Bellot, K. Langhans, & R. Schlichenmaier. (2005). Multi-line spectroscopy of dark-cored penumbral filaments. Astronomy and Astrophysics. 443(1). L7–L10. 30 indexed citations

6.

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

7.

Langhans, K., W. Schmidt, & Thomas Rimmelé. (2004). Diagnostic spectroscopy ofG-band brightenings in the photosphere of the sun. Astronomy and Astrophysics. 423(3). 1147–1157. 5 indexed citations

8.

Langhans, K. & W. Schmidt. (2002). Center-to-limb-variation of the G-band lines at 430.5 nm. Astronomy and Astrophysics. 382(1). 312–318. 7 indexed citations

9.

Langhans, K., W. Schmidt, & A. Tritschler. (2002). 2D-spectroscopic observations of $\vec G$-band bright structures in the solar photosphere. Astronomy and Astrophysics. 394(3). 1069–1076. 26 indexed citations

10.

Tritschler, A., W. Schmidt, K. Langhans, & T. Kentischer. (2002). High-resolution solar spectroscopy with TESOS – Upgrade from a double to a triple system. Solar Physics. 211(1-2). 17–29. 46 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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