TY - GEN
T1 - Using Plasma Clouds Produced by Dust Impacts on Parker Solar Probe to Search for Anomalous Dust Populations in the Inner Heliosphere
AU - Malaspina, David M.
AU - Mazurkiewicz, Avery
AU - Szalay, Jamey
AU - Lee-Bellows, Delaney
N1 - Publisher Copyright:
© 2025 USNC-URSI.
PY - 2025
Y1 - 2025
N2 - 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.
AB - 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.
UR - http://www.scopus.com/inward/record.url?scp=105001133276&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=105001133276&partnerID=8YFLogxK
U2 - 10.23919/USNC-URSINRSM66067.2025.10907163
DO - 10.23919/USNC-URSINRSM66067.2025.10907163
M3 - Conference contribution
AN - SCOPUS:105001133276
T3 - 2025 United States National Committee of URSI National Radio Science Meeting, USNC-URSI NRSM 2025 - Proceedings
SP - 29
BT - 2025 United States National Committee of URSI National Radio Science Meeting, USNC-URSI NRSM 2025 - Proceedings
PB - Institute of Electrical and Electronics Engineers Inc.
T2 - 2025 United States National Committee of URSI National Radio Science Meeting, USNC-URSI NRSM 2025
Y2 - 7 January 2025 through 10 January 2025
ER -