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Melrose, DB (1970) On the Theory of Type II and Type III Solar Radio Bursts. I. The Impossibility of Nonthermal Emission due to Combination Scattering Off Thermal Fluctuations. Australian Journal of Physics, 23 (5). 871pp. doi:10.1071/ph700871

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Reference TypeJournal (article/letter/editorial)
TitleOn the Theory of Type II and Type III Solar Radio Bursts. I. The Impossibility of Nonthermal Emission due to Combination Scattering Off Thermal Fluctuations
JournalAustralian Journal of Physics
AuthorsMelrose, DBAuthor
Year1970Volume23
Issue5
PublisherCSIRO Publishing
DOIdoi:10.1071/ph700871Search in ResearchGate
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Mindat Ref. ID10697819Long-form Identifiermindat:1:5:10697819:1
GUID0
Full ReferenceMelrose, DB (1970) On the Theory of Type II and Type III Solar Radio Bursts. I. The Impossibility of Nonthermal Emission due to Combination Scattering Off Thermal Fluctuations. Australian Journal of Physics, 23 (5). 871pp. doi:10.1071/ph700871
Plain TextMelrose, DB (1970) On the Theory of Type II and Type III Solar Radio Bursts. I. The Impossibility of Nonthermal Emission due to Combination Scattering Off Thermal Fluctuations. Australian Journal of Physics, 23 (5). 871pp. doi:10.1071/ph700871
In(1970) Australian Journal of Physics Vol. 23 (5) CSIRO Publishing

See Also

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

Melrose, DB (1970) On the Theory of Type II and Type III Solar Radio Bursts. II. Alternative Model. Australian Journal of Physics, 23 (5). 885pp. doi:10.1071/ph700885
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
Melrose, DB (1974) The Mechanism Responsible for 'Shadow' Type III Solar Radio Bursts. II. Absorption due to Ion Sound Turbulence. Australian Journal of Physics, 27 (2). 271pp. doi:10.1071/ph740271
(1966) Chains Of Type I Solar Radio Bursts. Australian Journal of Physics, 19 (5). 635pp. doi:10.1071/ph660635
Melrose, DB (1979) Propagation Effects on the Polarization of Pulsar Radio Emission. Australian Journal of Physics, 32 (2). 61pp. doi:10.1071/ph790061
Gopala Rao, UV (1965) The Polarization Structure of Type III Solar Radio Bursts. Australian Journal of Physics, 18 (3). 283pp. doi:10.1071/ph650283
Roberts, JA (1959) Solar Radio Bursts of Spectral Type II. Australian Journal of Physics, 12 (4). 327pp. doi:10.1071/ph590327
Melrose, D. B. (1975) Plasma emission due to isotropic fast electrons, and types I, II, and V solar radio bursts. Solar Physics, 43 (1). 211-236 doi:10.1007/bf00155154
Late AA Weiss, The (1965) The Nature and Velocity of the Sources of Type II Solar Radio Bursts. Australian Journal of Physics, 18 (2). 167pp. doi:10.1071/ph650167
Stewart, RT (1965) The Speed and Acceleration of the Sources of Type III And Type V Solar Radio Bursts Over Large Distances in the Corona. Australian Journal of Physics, 18 (1). 67pp. doi:10.1071/ph650067
Weiss, AA (1963) The Positions and Movements of the Sources of Solar Radio Bursts of Spectral Type II. Australian Journal of Physics, 16 (2). 240pp. doi:10.1071/ph630240
 
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