NASA NTRS · 20060036833
Extension of Coronal Structure Into Interplanetary Space
Abstract
The evolution of the solar corona and its imprint on the solar wind is investigated by comparing Ulysses radio occultation measurements of path-integrated electron density and density fluctuations in the heliocentric distance range of 21-32R(sub o) with simultaneous measurements of the solasr corona by the HAO Mauna Loa K-coronameter.
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Woo, Richard, Habbal, Shadia Rifai. 1996-01-01. Extension of Coronal Structure Into Interplanetary Space. https://ntrs.nasa.gov/citations/20060036833
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