| タイトル | Visibility related to backscatter at 1.54 micron |
| 本文（外部サイト） | http://hdl.handle.net/2060/19870000839 |
| 著者（英） | Larson, D. R.; Barber, T. L. |
| 著者所属（英） | Atmospheric Sciences Lab. |
| 発行日 | 1986-08-01 |
| 言語 | eng |
| 内容記述 | The lidar process was shown to have the necessary potential to fulfill the need for a remote measurement of visibility. Visibility can be inferred from a lidar return optical extinction. The wavelength 1.54 micron was chosen, being near the visible wavelength region and having a high eye safety threshol, 200,000 times higher than 1.06 micron; 1.54 is the erbium laser wavelength. This research utilized 105 measured height profiles of natural droplet size distributions data, taken in clouds, fog, and haze. These profiles were examined to determine the completeness of the droplet counting data. It was found that the particle spectrometer data were incomplete in the very light ford and haze so this portion of the data was eliminated. Utilizing the Mie theory, these droplet size distribution profiles were converted to backscatter at 1.54 micron and extinction in the visible region, 0.55 micron. Using Koschmeider's relationship, the extinction profiles were converted to visibility. The visibility and backscatter profiles were compared to develop a relationship between visibility and backscatter at 1.54 micron. |
| NASA分類 | ENVIRONMENT POLLUTION |
| レポートNO | 87N10272 |
| 権利 | No Copyright |
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