GH13*.1
Utilizing a Quasi-Specular Scattering Model to Enable Monte Carlo Simulation of Specular Meteor Radar Networks
James Monaco, John Marino, Scott Palo, University of Colorado Boulder, United States
Session:
GH13*: Meteors, Orbital Debris and Dusty Plasmas II Lecture
Track:
Special Sessions
Location:
Meadows A
Presentation Time:
Fri, 9 Jan, 15:20 - 15:40 MT (UTC -7)
Session Co-Chairs:
Trevor Hedges, Stanford University and Sigrid Elschot, Stanford University
Presentation
Discussion
Resources
No resources available.
Session GH13*
GH13*.1: Utilizing a Quasi-Specular Scattering Model to Enable Monte Carlo Simulation of Specular Meteor Radar Networks
James Monaco, John Marino, Scott Palo, University of Colorado Boulder, United States
GH13*.2: Toward a Polarimetric Theory of Meteor Radar Echoes
John Marino, Nicholas Rainville, Scott Palo, University of Colorado Boulder, United States
GH13*.3: Investigating Plasma Wave Signatures Due To Orbital Debris
Beatrice Evans, Naomi Maruyama, David Malaspina, University of Colorado, Boulder, United States
GH13*.4: Plasma signatures of small orbital debris in LEO
Gian Luca Delzanno, Pedro Resendiz, Justin Holmes, Salomon Janhunen, Los Alamos National Laboratory, United States
Contacts