Title: Martian
magnetic paleopoles: A geostatistical approach
Source: GEOPHYSICAL
RESEARCH LETTERS 32 (9): Art. No. L09201 MAY 3 2005
Document Type: Article
Language: English
Abstract: Various
attempts have been made to locate magnetic paleopoles on Mars by
modeling individual magnetic field anomalies. In this study, a quite
different approach, based on geostatistics, is taken. Discreet magnetic
sources form magnetic doublet anomalies in the magnetic field that tend
to align with the horizontal direction of magnetization. A
semivariogram of radial field polarities on Mars indicates that
magnetic field anomalies of opposite polarity tend to be separated by
14°. This phenomenon is interpreted to be due to the presence
of magnetic doublet anomalies in the field. Accordingly, the
autocovariances of the field polarity along longitudinal lines relative
to over 1000 trial paleopole locations were examined. Magnetic
paleopoles within about 50° of ( 230° E, 17° N)
and ( 50° E, 17° S) were found to best explain the
geostatistical structure of the polarity of the martian magnetic field.
KeyWords Plus: PALEOMAGNETIC
POLES; MARS; ANOMALIES; CRUST
Addresses: Sprenke
KF (reprint author), Univ Idaho, Dept Geol Sci, Moscow, ID 83844 USA
Univ Idaho, Dept Geol Sci, Moscow, ID 83844 USA
Publisher: AMER
GEOPHYSICAL UNION, 2000 FLORIDA AVE NW, WASHINGTON, DC 20009 USA
Subject Category: GEOSCIENCES,
MULTIDISCIPLINARY
IDS Number: 926TE
ISSN: 0094-8276