Abstract
A simple, iterative procedure to determine the optical depth components of the extinction optical depth measured by a solar radiometer is presented. Simulated data show that the iterative procedure improves the determination of the exponent of a Junge law particle size distribution. The determination of the optical depth due to aerosol scattering is improved as compared to a method which uses only two points from the extinction data. The iterative method was used to determine spectral optical depth components for 11-13 June 1988 during the MAC III experiment.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 91-101 |
| Number of pages | 11 |
| Journal | Remote Sensing of Environment |
| Volume | 32 |
| Issue number | 2-3 |
| DOIs | |
| State | Published - 1990 |
ASJC Scopus subject areas
- Soil Science
- Geology
- Computers in Earth Sciences