This map shows the geographic impact of H. Auraß'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 H. Auraß with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites H. Auraß more than expected).
This network shows the impact of papers produced by H. Auraß. 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 H. Auraß. The network helps show where H. Auraß may publish in the future.
Co-authorship network of co-authors of H. Auraß
This figure shows the co-authorship network connecting the top 25 collaborators of H. Auraß.
A scholar is included among the top collaborators of H. Auraß 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 H. Auraß. H. Auraß 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.
Warmuth, A., G. Mann, & H. Auraß. (2007). Constraining Electron Acceleration at a Standing Shock with HXR and Radio Observations. 31. 135.3 indexed citations
2.
Tomczak, M., et al.. (2007). Flare-Associated X-Ray Plasma Ejections and Radio Drifting Structures. 31. 125.1 indexed citations
Zlotnik, E. Ya., В. В. Зайцев, H. Auraß, G. Mann, & Axel Hofmann. (2003). Solar type IV burst spectral fine structures. Astronomy and Astrophysics. 410(3). 1011–1022.57 indexed citations
7.
Magdalenić, Jasmina, B. Vršnak, & H. Auraß. (2002). Solar type II radio bursts: emission from shock segments with a collapsing trap geometry?. ESASP. 1. 335–338.3 indexed citations
8.
Vršnak, B., Jasmina Magdalenić, H. Auraß, & G. Mann. (2002). Coronal and interplanetary magnetic fields inferred from band-splitting of type II bursts. ESASP. 1. 409–412.1 indexed citations
Mann, G., et al.. (1999). Coronal Transient Waves and Coronal Shock Waves. ESASP. 446. 477.21 indexed citations
12.
Vršnak, B., et al.. (1999). Energy Release Stages of the Complex Solar Flare of October 25, 1994. 23(1). 15–30.2 indexed citations
13.
Mann, G., H. T. Claßen, H. Auraß, et al.. (1998). Highly Energetic Electrons Accelerated by Coronal Shock Waves. Computers & Electrical Engineering.1 indexed citations
14.
Auraß, H., M. Dryer, M. D. Andrews, et al.. (1997). On Signatures of Nonthermal Particles During CME Acceleration. ESASP. 404. 183.3 indexed citations
15.
Mann, G., H. Auraß, H. T. Claßen, et al.. (1997). Shock Accelerated Electrons in the Corona. ESASP. 404. 543.1 indexed citations
16.
Sierks, H., W. Dröge, G. Mann, et al.. (1997). Electron Spectra and Associated Type II and Type III Radio Bursts of the July 9, 1996 Solar Event. International Cosmic Ray Conference. 1. 297.4 indexed citations
17.
Зайцев, В. В., H. Auraß, A. Kruger, & Greg Mann. (1994). On the origin of noise storm continuum depressions.. A&A. 291. 990–1000.1 indexed citations
18.
Auraß, H.. (1992). Radio observations of coronal and interplanetary type-II bursts : Solar activity. Annales Geophysicae. 10(6). 359–366.4 indexed citations
19.
Mann, G., et al.. (1992). Preliminary observations of solar type II bursts with the new radiospectrograph in Tremsdorf.. ESASP. 348. 129–132.2 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.