Extension of Coronal Structure into Interplanetary Space
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solar corona evolution solar wind Ulysses path-int↗
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Extension of Coronal Structure Into Interplanetary Space
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.
solar corona corona radio occultation Ulysses↗