Physics
Scientific paper
May 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agusmsa31a..07j&link_type=abstract
American Geophysical Union, Spring Meeting 2008, abstract #SA31A-07
Physics
2129 Interplanetary Dust, 6015 Dust, 6245 Meteors, 6952 Radar Atmospheric Physics (1220)
Scientific paper
In this work we use a semi-empirical model of the Micrometeor Input Function (MIF) together with meteor head- echo observations obtained with two High Power and Large Aperture (HPLA) radars to study the seasonal and geographical dependence of the meteoric flux in the upper atmosphere. The model includes an initial mass flux that is provided by six known meteor sources (i.e. orbital families of dust) as well as detailed modeling of meteoroid atmospheric entry and ablation physics. In addition, we use a simple ionization model to treat radar sensitivity issues by defining minimum electron volume density production thresholds required in the meteor head-echo plasma for detection. This simplified approach works well because we use observations from two radars with similar frequencies, but different sensitivities and locations. This methodology allows us the explore the initial input of particles and how it manifests in different parts of the MLT as observed by these instruments without the need to invoke more sophisticated plasma models, which are under current development. The comparisons between model predictions and radar observations show excellent agreement between diurnal, seasonal, and latitudinal variability of the detected meteor rate and radial velocity distributions, allowing us to understand how individual meteoroid populations contribute to the overall flux at a particular location and season.
Fentzke Jonathan T.
Janches Diego
Sparks James
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