Using Plasma Clouds Produced by Dust Impacts on Parker Solar Probe to Search for Anomalous Dust Populations in the Inner Heliosphere

David M. Malaspina, Avery Mazurkiewicz, Jamey Szalay, Delaney Lee-Bellows

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

The densest and most dynamic portion of the zodiacal dust cloud is Sunward of 1 AU. In this region, alpha meteoroids migrating sunward via Poynting-Robertson drag become dense enough for frequent collisions, outward propagating beta meteoroids are created, and dust grains can be efficiently sputtered and sublimated. Finally, the dust trails of comets and asteroids with perihelia under 1 AU stream through this region.

Original languageEnglish (US)
Title of host publication2025 United States National Committee of URSI National Radio Science Meeting, USNC-URSI NRSM 2025 - Proceedings
PublisherInstitute of Electrical and Electronics Engineers Inc.
Pages29
Number of pages1
ISBN (Electronic)9781946815200
DOIs
StatePublished - 2025
Event2025 United States National Committee of URSI National Radio Science Meeting, USNC-URSI NRSM 2025 - Boulder, United States
Duration: Jan 7 2025Jan 10 2025

Publication series

Name2025 United States National Committee of URSI National Radio Science Meeting, USNC-URSI NRSM 2025 - Proceedings

Conference

Conference2025 United States National Committee of URSI National Radio Science Meeting, USNC-URSI NRSM 2025
Country/TerritoryUnited States
CityBoulder
Period1/7/251/10/25

All Science Journal Classification (ASJC) codes

  • Radiation
  • Computer Networks and Communications
  • Control and Optimization
  • Modeling and Simulation
  • Instrumentation

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