Figure 3 from Modeling the Altitude Distribution of Meteor Head Echoes Observed with HPLA Radars: Implications for the Radar Detectability of Meteoroid Populations

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

Modeling the Altitude Distribution of Meteor Head Echoes Observed with HPLA Radars: Implications for the Radar Detectability of Meteoroid Populations

Authors: N. Swarnalingam, D. Janches, J. D. Carrillo-Sanchez, P. Pokorny, J. M. C. Plane, Z. Sternovsky, and D. Nesvorny

2019 The Astronomical Journal 157 179.

Provider: AAS Journals

Caption: Figure 3.

Comparison of weighted velocity distributions of JFCs, HTCs, and OCCs, predicted to be detected by the Arecibo (AO), PFISR (PF), and MU radars when the detection model described in Janches et al. (2017) is applied to each radar.

Other Images in This Article

Copyright and Terms & Conditions