GH4*.1
Predicting the Spectral Intensity of Hypervelocity Impact Plasma Emissions
Cole Robins, Nicolas Lee, Sigrid Elschot, Stanford University, United States
Session:
GH4*: Meteors Orbital Debris and Dusty Plasmas Lecture
Track:
Special Sessions
Location:
Room 200
Presentation Time:
Wed, 8 Jan, 13:30 - 13:50 MT (UTC -7)
Session Co-Chairs:
Alex Fletcher, and Paul Bernhardt,
Presentation
Discussion
Resources
No resources available.
Session GH4*
GH4*.1: Predicting the Spectral Intensity of Hypervelocity Impact Plasma Emissions
Cole Robins, Nicolas Lee, Sigrid Elschot, Stanford University, United States
GH4*.2: Track After Detection of Inert Space Objects in Conjunction with Satellite-Based Plasma Wave Sensors
Paul Bernhardt, University of Alaska Fairbanks, United States; Bengt Eliasson, University of Strathclyde, United Kingdom; Wayne Scales, Andrew Howarth, Virginia Tech, United States; Lauchie scott, DRDC Ottawa Research Centre, Canada; Andrew Foss, univeristy of cal, Canada
GH4*.3: Simultaneous Observation of a Daytime Arietids Meteor Head Echo at VHF and UHF Frequencies
Trevor Hedges, Stanford University, United States; Alex Green, Boston University, United States; Nicolas Lee, Sigrid Elschot, Stanford University, United States; Meers Oppenheim, Boston University, United States
GH4*.4: Using Plasma Clouds Produced by Dust Impacts on Parker Solar Probe to Search for Anomalous Dust Populations in the Inner Heliosphere
David Malaspina, Avery Mazurkiewicz, University of Colorado, Boulder, United States; Jamey Szalay, Princeton University, United States; Delaney Lee-Bellows, University of Colorado, Boulder, United States
GH4*.5: Towards resolving the wake structure of a dust grain in plasma with wave kinetic models
Michael Kwara, Sigrid Elschot, Stanford University, United States
Contacts