作者: R. Woo , J.W. Armstrong
DOI: 10.1016/B978-0-08-042049-3.50070-3
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摘要: ABSTRACT A study of large-scale structure in the inner heliosphere based on unique and extensive Pioneer Venus Doppler scintillation data has been initiated. Preliminary results include first observation corotating stream inside 35 Ro. Results variations scintillations with solar cycle heliocentric distance, their implications terms wind mass flux density, are discussed.