Abstract
It is shown that non-parallel density and temperature gradients can produce magnetic fields which can account for the asteroid Gaspra surface magnetic field of about one Gauss.
Export citation and abstract BibTeX RIS
Click here to close this panel.
R Bingham1 and J M Dawson2
Published under licence by IOP Publishing Ltd
,
,
Citation R Bingham and J M Dawson 1999 Phys. Scr. 1999 137
DOI 10.1238/Physica.Topical.082a00137