Radio tracking of a white-light coronal mass ejection from solar corona to interplanetary medium

被引：34

作者：

Reiner, MJ ^{[1
]}

Kaiser, ML

Plunkett, SP

Prestage, NP

Manning, R

机构：

[1] Raytheon ITSS, Lanham, MD 20706 USA

[2] NASA, Goddard Space Flight Ctr, Extraterr Phys Lab, Greenbelt, MD 20771 USA

[3] USN, Res Lab, Univ Space Res Assoc, Washington, DC 20375 USA

[4] Culgoora Solar Observ, IPS Radio & Space Serv, Narrabri, NSW 2390, Australia

[5] Observ Paris, DESPA, F-92195 Meudon, France

来源：

ASTROPHYSICAL JOURNAL | 2000年 / 529卷 / 01期

基金：

美国国家科学基金会;

关键词：

solar-terrestrial relations; Sun : activity; Sun : corona; Sun : flares; Sun : radio radiation;

D O I：

10.1086/312446

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

For a solar flare/coronal mass ejection (CME) event on 1999 May 3, type II radio emissions were observed from the metric through the hectometric wavelength regimes. By comparing the dynamics of the CME with that implied by the frequency range and frequency drift rates of the type II radio emissions, it is concluded that the decametric-hectometric type IT radio emissions were associated with the CME. The dynamics implied by the metric type II radio burst suggest a distinct coronal shock, associated with the flare, which only produced radio emissions in the low corona.

引用

页码：L53 / L56

页数：4

共 15 条

[1]

BOUGERET JL, 1984, SOL PHYS, V90, P401, DOI 10.1007/BF00173965

[2] WAVES - THE RADIO AND PLASMA-WAVE INVESTIGATION ON THE WIND SPACECRAFT [J].