Line formation in solar granulation
The solar photospheric oxygen abundance has been determined from [O I], O I, OH vibration-rotation and OH pure rotation lines by means of a realistic time-dependent, 3D, hydrody...
Publications
2 shownLine formation in solar granulation
The solar photospheric carbon abundance has been determined from [C i], C i, CH vibration-rotation, CH A-X electronic and C2 Swan electronic lines by means of a time-dependent, ...
Frequent Co-Authors
Researcher Info
- h-index
- 2
- Publications
- 2
- Citations
- 884
- Institution
- The University of Texas at Austin
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Impact Metrics
h-index
2
h-index: Number of publications with at least h citations each.