On the origin of radio emissions associated with the January 6–11, 1997, CME
- 15 July 1998
- journal article
- Published by American Geophysical Union (AGU) in Geophysical Research Letters
- Vol. 25 (14) , 2493-2496
- https://doi.org/10.1029/98gl00138
Abstract
No abstract availableThis publication has 12 references indexed in Scilit:
- A magnetic cloud containing prominence material: January 1997Journal of Geophysical Research, 1998
- Location of the radio emitting regions of interplanetary shocksJournal of Geophysical Research, 1992
- Characteristics of interplanetary type II radio emission and the relationship to shock and plasma propertiesJournal of Geophysical Research, 1989
- Shock-associated kilometric radio emission and solar metric type II burstsSolar Physics, 1989
- Energetic interplanetary shocks, radio emission, and coronal mass ejectionsJournal of Geophysical Research, 1987
- The evolution of interplanetary shocksJournal of Geophysical Research, 1985
- Type II solar radio bursts, interplanetary shocks, and energetic particle eventsThe Astrophysical Journal, 1984
- Solar radio burst and in situ determination of interplanetary electron densitySolar Physics, 1984
- Type II solar radio events observed in the interplanetary mediumSolar Physics, 1982
- Radio evidence for shock acceleration of electrons in the solar coronaGeophysical Research Letters, 1981