Astronomy and Astrophysics – Astrophysics
Scientific paper
Sep 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26a...289..957h&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 289, no. 3, p. 957-971
Astronomy and Astrophysics
Astrophysics
23
Interplanetary Medium, Magnetohydrodynamic Waves, Plasma Frequencies, Propagation Modes, Radio Observation, Type 3 Bursts, Data Correlation, Electron Energy, Harmonic Analysis, Radio Spectra, Spectrum Analysis, Ulysses Mission
Scientific paper
We study a set of solar type 3 radio bursts where the emission is visible from the high-frequency limit of the radio astronomy receiver of the Ulysses Unified Radio and Plasma wave (URAP) experiment down to low frequencies, sometimes near the plasma frequency, and where Langmuir wave spikes are recorded by the radio and/or plasma receivers. Our results pose questions regarding radio emission by Langmuir waves. When Langmuir waves are observed, why is it only sometimes that radio radiation is emitted at the fundamental? Put another way, why is there often a gap or a cutoff in the radiation at a frequency well above the plasma frequency? In the few cases where the radiation at times of Langmuir wave spikes is at the harmonic, why is there no fundamental?
Dulk George A.
Hoang Sang
Leblanc Yolanda
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