Observations of solar radio bursts from meter to kilometer wavelengths

Conference · Sun Jan 01 00:00:00 EST 1984 · Adv. Space Res.; (United States)

OSTI ID:5477148

Kundu, M R; Stone, R G

New results obtained with the Clark Lake multifrequency radioheliograph at meter-decameter wavelengths and from satellite multifrequency directive observations at hectometer and kilometer wavelengths are reviewed. Evidence is presented that type III electrons propagate in dense coronal streamers and that frequently observed microbursts (presumably type III) at meter-decameter wavelengths are due to plasma radiation. Observations of hectometer and kilometer type III radio storms which reveal information about active region structures, the interplanetary magnetic field configuration, and solar wind acceleration are discussed. Kilometer type II bursts and interactions between type III electrons and interplanetary shocks are examined, and some new results on shock-associated events are presented. 23 references.

• Research Organization: Maryland Univ., College Park
• OSTI ID: 5477148
• Report Number(s): CONF-8406167-
• Journal Information: Adv. Space Res.; (United States), Vol. 4; Conference: 25. plenary session of COSPAR, Graz, Austria, 25 Jun 1984
• Country of Publication: United States
• Language: English

Related Subjects

71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
SOLAR RADIO BURSTS
LONG WAVE RADIATION
SOLAR CORONA
SOLAR ELECTRONS
SOLAR WIND
ATMOSPHERES
ELECTROMAGNETIC RADIATION
ELECTRONS
ELEMENTARY PARTICLES
FERMIONS
LEPTONS
RADIATIONS
RADIOWAVE RADIATION
SOLAR ACTIVITY
SOLAR PARTICLES
SOLAR RADIATION
STELLAR ATMOSPHERES
STELLAR CORONAE
STELLAR RADIATION
640104* - Astrophysics & Cosmology- Solar Phenomena