Abstract
A method for combining nadir observations of emission features in the upper atmosphere with the result of a tomographic inversion of limb brightness measurements is presented. Simulated and actual results are provided, and error sensitivity is investigated.
| Original language | English |
|---|---|
| Pages (from-to) | 4134-4140 |
| Number of pages | 7 |
| Journal | Applied Optics |
| Volume | 24 |
| Issue number | 23 |
| DOIs | |
| State | Published - Dec 1985 |
| Externally published | Yes |