Skip to main content
OSTI.GOVU.S. Department of Energy Office of Scientific and Technical Information
U.S. Department of Energy
Office of Scientific and Technical Information
 

Data for "Propagation of EMIC Waves from Shabansky Orbits in the Dayside Magnetosphere"

Dataset ·
DOI:https://doi.org/10.34770/e3m1-rs25· OSTI ID:2589019
 [1];  [1];  [2];  [1];  [3];  [4];  [5];  [6];  [2]
  1. Princeton Plasma Physics Laboratory
  2. Andrews University
  3. Southwest Research Institute
  4. Kyung Hee University, Korea
  5. Augsburg University
  6. New Jersey Institute of Technology
+ Show Author Affiliations

Full-wave simulations of electromagnetic ion cyclotron waves in a non-dipole compressed magnetic field have been conducted using the Petra-M simulation code. The manuscript investigates the effect of misalignment of the Faraday screen and electron density in the scrape-off layer on the excitation and propagation of fast helicon and slow mode waves.

Research Organization:
Princeton Plasma Physics Laboratory
Sponsoring Organization:
National Research Foundation of Korea ; NASA; NSF; MMS mission; United States Department of Energy
DOE Contract Number:
AC02-05CH11231; AC02-09CH11466; SC0024369
OSTI ID:
2589019
Country of Publication:
United States
Language:
English

Cited By (1)

Propagation of EMIC Waves From Shabansky Orbits in the Dayside Magnetosphere journal February 2025

Similar Records

Propagation of EMIC Waves From Shabansky Orbits in the Dayside Magnetosphere
Journal Article · Tue Feb 11 23:00:00 EST 2025 · Geophysical Research Letters · OSTI ID:2514550

Related Subjects

Magnetosphere: outer
Plasma waves and instabilities
wave interactions