The Venus Solar Wind Interaction — Is It Purely Ionospheric?

Details The Venus Solar Wind Interaction — Is It Purely Ionospheric? The Venus Solar Wind Interaction — Is It Purely Ionospheric?

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1521l&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1521

Physics

Scientific paper

Reanalysis of magnetic fields observed on Pioneer Venus Orbiter suggests
the presence of a persistent hemispheric radial magnetic field bias in
the wake above ~250 km. We use a model to ask how a planet-centered weak
dipole would manifest itself.

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