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Gubchenko, V.M., Zaitsev, V.V. (1983) The source model of low-energy electrons responsible for type I and type III radio noise storms. Solar Physics, 89 (2). doi:10.1007/bf00217258

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Reference TypeJournal (article/letter/editorial)
TitleThe source model of low-energy electrons responsible for type I and type III radio noise storms
JournalSolar Physics
AuthorsGubchenko, V.M.Author
Zaitsev, V.V.Author
Year1983 (December)Volume89
Issue2
PublisherSpringer Science and Business Media LLC
DOIdoi:10.1007/bf00217258Search in ResearchGate
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Mindat Ref. ID8917692Long-form Identifiermindat:1:5:8917692:2
GUID0
Full ReferenceGubchenko, V.M., Zaitsev, V.V. (1983) The source model of low-energy electrons responsible for type I and type III radio noise storms. Solar Physics, 89 (2). doi:10.1007/bf00217258
Plain TextGubchenko, V.M., Zaitsev, V.V. (1983) The source model of low-energy electrons responsible for type I and type III radio noise storms. Solar Physics, 89 (2). doi:10.1007/bf00217258
In(1983, December) Solar Physics Vol. 89 (2) Springer Science and Business Media LLC

See Also

These are possibly similar items as determined by title/reference text matching only.

Gubchenko, V.M., Zaitsev, V.V. (1979) On proton and electron acceleration by shock waves during large solar flares. Solar Physics, 63 (2). doi:10.1007/bf00174539
Goldman, MartinV. (1983) Progress and problems in the theory of type III solar radio emission. Solar Physics, 89 (2). doi:10.1007/bf00217259
Gurnett, D. A., Frank, L. A. (1976) The relationship of electron plasma oscillations to type III radio emissions and low-energy solar electrons. Solar Physics, 46 (2). 459 doi:10.1007/bf00149868
Fainberg, Joseph, Stone, R. G. (1970) Type III solar radio burst storms observed at low frequencies. Solar Physics, 15 (2). 433-445 doi:10.1007/bf00151850
Fainberg, Joseph, Stone, R. G. (1971) Type III solar radio burst storms observed at low frequencies. Solar Physics, 17 (2). 392-401 doi:10.1007/bf00150042
Frank, L. A., Gurnett, D. A. (1972) Direct observations of low-energy solar electrons associated with a type III solar radio burst. Solar Physics, 27 (2). 446-465 doi:10.1007/bf00153116
Kane, S. R. (1972) Evidence for a common origin of the electrons responsible for the impulsive X-ray and type III radio bursts. Solar Physics, 27 (1). 174-181 doi:10.1007/bf00151781
Brueckner, G. E. (1983) Type I noise storms and the structure of the extreme ultraviolet corona. Solar Physics, 85 (2). 243-265 doi:10.1007/bf00148653
Duncan, R. A. (1983) Dynamic behaviour of the K-corona above a type I radio source. Solar Physics, 89 (1). 63-76 doi:10.1007/bf00211953
Fainberg, Joseph, Stone, R. G. (1970) Type III solar radio burst storms observed at low frequencies. Solar Physics, 15 (1). 222-233 doi:10.1007/bf00149487
Melrose, DB (1974) The Mechanism Responsible for 'Shadow' Type III Solar Radio Bursts. I. Absorption due to Langmuir Turbulence. Australian Journal of Physics, 27 (2). 259pp. doi:10.1071/ph740259
 
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