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Thomas E. Cravens is an American space physicist and Professor Emeritus in the Department of Physics and Astronomy at the University of Kansas. He is known for developing the widely accepted model explaining the emission of X-rays from comets, a phenomenon discovered unexpectedly in 1996.
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university cravens physics space solar wind planetary cometary x-ray emission comets model x-rays state research kansas mars saturn doi 10
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| Thomas E. Cravens | Alma mater | Harvard University (Ph.D.) State University of New York at Stony Brook (B.A.) | 1.00 | infobox |
| Thomas E. Cravens | Awards | Fellow of the AAAS (2018) Higuchi Award (2005) Fellow of AGU (2001) AGU Editors' Citation for Excellence in Refereeing (2003) | 1.00 | infobox |
| Thomas E. Cravens | Doctoral advisor | Alex Dalgarno | 1.00 | infobox |
| Thomas E. Cravens | Fields | Space physics, Planetary science | 1.00 | infobox |
| Thomas E. Cravens | Known for | Cometary X-ray emission model Solar wind interactions with planets and comets | 1.00 | infobox |
| Thomas E. Cravens | Workplaces | University of Kansas University of Michigan | 1.00 | infobox |
| O6 | instance of | The solar wind contains ions | 0.80 | text |
| NASA Astrophysics Data System. | instance of | 00051-8.A more extensive list of publications is available through databases | 0.80 | text |
| Google Scholar | instance of | 00051-8.A more extensive list of publications is available through databases | 0.80 | text |
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