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Latitudinal Variation of Solar Wind Speed and Mass Flux in the Acceleration Region of the Solar Wind during Solar Minimum Inferred from Spectral Broadening measurements

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dc.contributor.author Woo, R. en_US
dc.contributor.author Goldstein, R. en_US
dc.date.accessioned 2004-10-06T05:20:29Z
dc.date.available 2004-10-06T05:20:29Z
dc.date.issued 1993-12-06 en_US
dc.identifier.citation EOS, American Geophysical Union en_US
dc.identifier.citation San Francisco, California, USA en_US
dc.identifier.clearanceno 93-1674 en_US
dc.identifier.uri http://hdl.handle.net/2014/35945
dc.description.abstract In this paper, we use an aggregate of S-band 2.3 GHz (13 cm) spectral broadening observations conducted during solar minimum conditions by the Mariner 4, Pioneer 10, Mariner 10, Helios 1 & 2 and Viking spacecraft to infer the first measurements of the latitudinal variation of solar wind speed and mass flux in the acceleration region of the solar wind at 3-8 R<sub>o</sub>. en_US
dc.format.extent 62800 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other latitudinal variation of solar wind mass flux in accelleration en_US
dc.title Latitudinal Variation of Solar Wind Speed and Mass Flux in the Acceleration Region of the Solar Wind during Solar Minimum Inferred from Spectral Broadening measurements en_US


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