Solar flares, type III radio bursts, coronal mass ejections, and energetic particles
Top Cited Papers
Open Access
- 22 October 2002
- journal article
- solar and-heliospheric-physics
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 107 (A10) , SSH 14-1-SSH 14-19
- https://doi.org/10.1029/2001ja000320
Abstract
No abstract availableKeywords
This publication has 43 references indexed in Scilit:
- The correlation between solar energetic particle peak intensities and speeds of coronal mass ejections: Effects of ambient particle intensities and energy spectraJournal of Geophysical Research, 2001
- Calibration of low-frequency radio telescopes using the galactic background radiationAstronomy & Astrophysics, 2001
- Acceleration of electrons at type II shock fronts and production of shock‐accelerated type III burstsJournal of Geophysical Research, 2000
- On the Solar Origin of Complex Type III–like Radio Bursts Observed at and below 1 MHzThe Astrophysical Journal, 2000
- Soft X-ray emissions, meter-wavelength radio bursts, and particle acceleration in solar flaresThe Astrophysical Journal, 1988
- The composition of solar energetic particlesThe Astrophysical Journal, 1986
- Type II solar radio bursts, interplanetary shocks, and energetic particle eventsThe Astrophysical Journal, 1984
- Radio burst characteristics of solar proton flaresThe Astrophysical Journal, 1982
- Radio evidence for shock acceleration of electrons in the solar coronaGeophysical Research Letters, 1981
- Solar Radio Bursts of Spectral Type IIAustralian Journal of Physics, 1959