Journal article
ULYSSES-GALILEO OBSERVATIONS OF TYPE-III RADIO-BURSTS AND ASSOCIATED IN-SITU ELECTRONS AND LANGMUIR-WAVES
Space science reviews, Vol.72(1-2), pp.261-266
04/01/1995
DOI: 10.1007/BF00768789
Abstract
Both the Ulysses and Galileo spacecraft detected energetic electrons and Langmuir waves that were associated with a type III radio burst on 10 December 1990. At the time of these observations, these spacecraft were in the ecliptic plane and separated by 0.4 AU, with Galileo near the Earth at 1 AU and Ulysses at 1.36 AU. From the measured electron arrival times, the propagation path lengths of the electrons to both Ulysses and Galileo were estimated to be significantly longer than the length of the Parker spiral. These long path lengths are interpreted as due to draping of the interplanetary magnetic field lines around a CME. The onset times of the Langmuir waves at Ulysses and Galileo coincided with the estimated arrival time of the 9 keV and 14 keV electrons, respectively.
Details
- Title: Subtitle
- ULYSSES-GALILEO OBSERVATIONS OF TYPE-III RADIO-BURSTS AND ASSOCIATED IN-SITU ELECTRONS AND LANGMUIR-WAVES
- Creators
- M J ReinerK A AndersonE RoelofT ArmstrongG B HospodarskyJ FainbergR G StoneL LanzerottiD A GurnettJ L PhillipsR Forsyth
- Resource Type
- Journal article
- Publication Details
- Space science reviews, Vol.72(1-2), pp.261-266
- Publisher
- Springer Nature
- DOI
- 10.1007/BF00768789
- ISSN
- 0038-6308
- eISSN
- 1572-9672
- Number of pages
- 6
- Language
- English
- Date published
- 04/01/1995
- Academic Unit
- Physics and Astronomy
- Record Identifier
- 9984455546202771
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