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.
Original language | English |
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Pages (from-to) | 137 |
Number of pages | 1 |
Journal | Physica Scripta |
Volume | 1999 |
Issue number | T82 |
DOIs | |
Publication status | Published - 1999 |
Keywords
- asteroids
- plasma properties