Sabine Richling
- Astronomy and Astrophysics top 5%
- Astrophysics and Star Formation Studies 9
- Stellar, planetary, and galactic studies 5
- Galaxies: Formation, Evolution, Phenomena 5
- Astro and Planetary Science 4
- Instrumentation top 10%
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- Advanced Optical Network Technologies 3
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- Parallel Computing and Optimization Techniques 3
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- Distributed and Parallel Computing Systems 3
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- Advanced Chemical Physics Studies 2
- Co-authors
- H. W. YorkeGuido KanschatNikolai V. KryzhevoiI. AppenzellerD. MehlertStefan NollC. TapkenJ. Heidt
- Partner nations
- GermanyFranceUnited States
In The Last Decade
Sabine Richling
19 papers receiving 305 citations
Peers
Comparison fields: 5 of 38
- Astronomy and Astrophysics 235
- Instrumentation 43
- Spectroscopy 41
- Acoustics and Ultrasonics 2
- Nuclear and High Energy Physics 28
Countries citing papers authored by Sabine Richling
This map shows the geographic impact of Sabine Richling'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 Sabine Richling with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites Sabine Richling more than expected).
Fields of papers citing papers by Sabine Richling
This network shows the impact of papers produced by Sabine Richling. 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 Sabine Richling. The network helps show where Sabine Richling may publish in the future.
Co-authorship network
The 20 scholars most cited alongside Sabine Richling, linked wherever they have co-authored with each other. Click a name or a connecting line to browse the papers they share.
All Works
| # | Work | ||
|---|---|---|---|
| 1 | 2015 | 1 | |
| 2 | 2012 | 1 | |
| 3 | 2011 | 2 | |
| 4 | 2011 | 4 | |
| 5 | 2010 | 5 | |
| 6 | 2010 | 3 | |
| 7 | 2008 | 9 | |
| 8 | 2007 | 64 | |
| 9 | 2004 | 17 | |
| 10 | 2003 | 10 | |
| 11 | 2003 | 2 | |
| 12 | The effects of winds and photoionization on the evolution of protostellar disks | 2002 | 1 |
| 13 | 2002 | 15 | |
| 14 | 2001 | 61 | |
| 15 | 2000 | 77 | |
| 16 | 2000 | 34 | |
| 17 | 1998 | 1 | |
| 18 | Photoevaporation of protostellar disks IV. Externally illuminated disks | 1998 | 2 |
| 19 | 1997 | 3 |
About Sabine Richling
Sabine Richling is a scholar working on Astronomy and Astrophysics, Hardware and Architecture and Computer Networks and Communications, having authored 19 papers that have together received 312 indexed citations. Recurring topics across this work include Astrophysics and Star Formation Studies (9 papers), Stellar, planetary, and galactic studies (5 papers), Galaxies: Formation, Evolution, Phenomena (5 papers), Astro and Planetary Science (4 papers), Advanced Optical Network Technologies (3 papers), Parallel Computing and Optimization Techniques (3 papers), Distributed and Parallel Computing Systems (3 papers) and Advanced Chemical Physics Studies (2 papers). The work is most often cited by research in Astronomy and Astrophysics (235 citations), Instrumentation (43 citations) and Spectroscopy (41 citations). Sabine Richling has collaborated with scholars based in Germany, France and United States. Frequent co-authors include H. W. Yorke, Guido Kanschat, Nikolai V. Kryzhevoi, I. Appenzeller, D. Mehlert, Stefan Noll, C. Tapken, J. Heidt, Heinz Kredel and H. Zinnecker.
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.