HR: 16:30h
AN: GP34A-03 [Abstracts]
TI: Inclination Error Correction In Red Beds: Is It Possible ?
AU: de Groot, L V
EM: l.v.degroot@phys.uu.nl
AF: Paleomagnetic Laboratory Fort Hoofddijk, Utrecht University, Budapestlaan 17, Utrecht,
3584 CD, Netherlands
AU: Haldan, M M
EM: haldan@geo.uu.nl
AF: Paleomagnetic Laboratory Fort Hoofddijk, Utrecht University, Budapestlaan 17, Utrecht,
3584 CD, Netherlands
AU: * Langereis, C G
EM: langer@geo.uu.nl
AF: Paleomagnetic Laboratory Fort Hoofddijk, Utrecht University, Budapestlaan 17, Utrecht,
3584 CD, Netherlands
AB:
Highly detailed records - including processing of hundreds of samples - have been obtained
from red beds in southern France, in the Dôme de Barrot and Lodève basins. The main purpose
was to sample and determine paleosecular variation (PSV) - over sufficient time - during the Permian
Superchron. We compared our records with older and earlier published literature data, and generally find good
agreement.
Since (hematite bearing) red beds are famous for their inclination error, we tried to correct our distributions using
two independent methods. One method is using a PSV model (TK03.GAD; Tauxe and Kent, 2004) which - not
surprisingly for such low latitudes - gives no significant correction on the distributions that
sufficiently sample PSV. In addition, our data are in very good agreement with published APWP data, giving
confidence in the recording qualities of these red beds, at least at paleoequatorial latitudes.
Another method is to correct the inclination via an approach (the "a-
factor"of Tan and Kodama, 2002) that uses the anisotropies of the magnetic susceptibility
and of laboratory acquired (anhysteretic or isothermal) remanence.
To this end, we sampled single layers, that we assumed to record - approximately - one
single occurrence of PSV. A model approach was used to estimate the a-factor, rather than determining this
parameter from laboratory experiments. We also used TK03.GAD on a large distribution (N=~200) of these single
layer samples.
This yielded interesting results. In one case a positive inclination was corrected - via the a-
factor model - to a negative inclination, and in an another case the Permian red beds were corrected
- using the TK03.GAD model - to a position at the latitude of the Netherlands, in contrast to
their assumed paleo-equatorial position.
We discuss the various merits of these different and independent methods for inclination error correction in these
(and other) red bed sequences.
DE: 1518 Magnetic fabrics and anisotropy
DE: 1522 Paleomagnetic secular variation
DE: 1560 Time variations: secular and longer
SC: Geomagnetism and Paleomagnetism [GP]
MN: 2007 Fall Meeting