Distortion of meteor count rates due to cosmic radio noise and atmospheric particularities

Thumbnail Image
Date
2010
Volume
8
Issue
Journal
Series Titel
Book Title
Publisher
Göttingen : Copernicus
Link to publishers version
Abstract

The determination of the meteoroid flux is still a scientifically challenging task. This paper focusses on the impact of extraterrestrial noise sources as well as atmospheric phenomena on the observation of specular meteor echoes. The effect of cosmic radio noise on the meteor detection process is estimated by computing the relative difference between radio loud and radio quiet areas and comparing the monthly averaged meteor flux for fixed signal-to-noise ratios or fixed electron line density measurements. Related to the cosmic radio noise is the influence of D-layer absorption or interference with sporadic E-layers, which can lead to apparent day-to-day variation of the meteor flux of 15-20%. © 2010 Author(s).

Description
Keywords
Atmospheric phenomena, Count rates, Meteor detection, Meteor echos, Meteoroid flux, Noise source, Quiet areas, Radio noise, Atmospheric electricity, Cosmology, D region, E region, Meteor impacts, Radio astronomy
Citation
Stober, G., Jacobi, C., & Keuer, D. (2010). Distortion of meteor count rates due to cosmic radio noise and atmospheric particularities. 8. https://doi.org//10.5194/ars-8-237-2010
License
CC BY 3.0 Unported