Abstract
In meteor photography the velocity of meteors is generally obtained from a chopper which blocks periodically the incident light beam in front of the camera lens. In this paper I examine modulation of the meteor trail instead with a sinodial function and use frequency analysis to compute accurately the mean atmospheric velocity.
| Original language | Undefined/Unknown |
|---|---|
| Pages (from-to) | 205-208 |
| Number of pages | 4 |
| Journal | Earth, Moon, and Planets |
| Volume | 102 |
| Issue number | 1-4 |
| Publication status | Published - 2008 |
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