Energetic particle propagation in the inner heliosphere as deduced from low‐frequency (<100 kHz) observations of type III radio bursts
- 21 May 2003
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 108 (A5)
- https://doi.org/10.1029/2002ja009488
Abstract
No abstract availableKeywords
This publication has 19 references indexed in Scilit:
- Solar flares, type III radio bursts, coronal mass ejections, and energetic particlesJournal of Geophysical Research, 2002
- Latitudinal heliospheric magnetic field: Stochastic and causal componentsJournal of Geophysical Research, 2001
- On the Origin of Impulsive Electron Events Observed at 1 AUThe Astrophysical Journal, 1999
- RADIO EMISSION FROM SOLAR FLARESAnnual Review of Astronomy and Astrophysics, 1998
- Electron beams and radio waves of solar Type III burstsJournal of Geophysical Research, 1998
- Observation of an impulsive solar electron event extending down to ∼0.5 keV energyGeophysical Research Letters, 1996
- The low radio frequency limit of solar type III bursts: Ulysses observations in and out of the eclipticGeophysical Research Letters, 1995
- Large-Scale Interplanetary Magnetic Field Configuration Revealed by Solar Radio BurstsScience, 1995
- The composition of solar energetic particlesThe Astrophysical Journal, 1986
- Harmonics in the Spectra of Solar Radio DisturbancesAustralian Journal of Physics, 1954