TY - JOUR
T1 - High-resolution record of geomagnetic secular variation from late Pleistocene Lake Lisan sediments (paleo Dead Sea)
AU - Marco, Shmuel
AU - Ron, Hagai
AU - McWilliams, Michael O.
AU - Stein, Mordechai
N1 - Funding Information:
This project is part of a large-scale research on the geology of the Lisan Formation conducted by Abraham Starinsky (A.S.), the Institute of Earth Sciences, the Hebrew University of Jerusalem. It was funded by the US–Israel Binational Science Foundation grant #9200346 to A.S., M.O.M., H.R., and M.S. We are grateful to Amotz Agnon, Alexandra Schramm, and Steve Goldstein for constructive and fruitful discussions and help in fieldwork. Thanks to Ori Gonen and Revital Ken-Tor for assistance in operating the magnetometer and in fieldwork, and to Rami Weinberger, Yuval Bartov, Ofra Klein, Noya Shilony, Amir Sagy, and Malka Machlus, for help in the field. Reviews by Gillian Turner and Niels Abrahamsen are highly appreciated. [RV]
PY - 1998/9
Y1 - 1998/9
N2 - We measured geomagnetic secular variation in Lake Lisan sediments (paleo Dead Sea). More than 1500 oriented samples were collected from a 27.3-m section of alternating aragonite and detritus laminae in the Dead Sea basin ranging in age from 67 to 32 ka. The natural remanent magnetization (NRM) is carried by titanomagnetite in the detrial laminae whereas the aragonite is diamagnetic. The NRM is very stable and was acquired several hundred years after deposition. The mean direction of 878 horizons is D = 005°, I = 45°(α95 = 1°; κ = 22). We observed three modes of directional geomagnetic variation as a function of (and by inference, time): very rapid inter-sample changes, slow variation in mean direction, and inclination shallowing of about 1°/m. The overall rate of change in direction is 0.57 ± 0.57°/year, not significantly different from zero. For about 83% of the record the rate of change is less than 1°/year and comparable to historical values. High rates of change are observed more frequently in the Lisan than in historical records, and peak rates are up to ten times faster. A smoothed curve resulting in a maximum rate of change of 0.66°/year and a mean 0.10 ± 0.10°/year may be a more realistic representation of the field behavior. No reverse NRMs were observed, but geomagnetic field excursions may be present where the VGPs deviate by more than 40°from the geographic north at about 52 and 41 ka; the latter may represent the Laschamp event.
AB - We measured geomagnetic secular variation in Lake Lisan sediments (paleo Dead Sea). More than 1500 oriented samples were collected from a 27.3-m section of alternating aragonite and detritus laminae in the Dead Sea basin ranging in age from 67 to 32 ka. The natural remanent magnetization (NRM) is carried by titanomagnetite in the detrial laminae whereas the aragonite is diamagnetic. The NRM is very stable and was acquired several hundred years after deposition. The mean direction of 878 horizons is D = 005°, I = 45°(α95 = 1°; κ = 22). We observed three modes of directional geomagnetic variation as a function of (and by inference, time): very rapid inter-sample changes, slow variation in mean direction, and inclination shallowing of about 1°/m. The overall rate of change in direction is 0.57 ± 0.57°/year, not significantly different from zero. For about 83% of the record the rate of change is less than 1°/year and comparable to historical values. High rates of change are observed more frequently in the Lisan than in historical records, and peak rates are up to ten times faster. A smoothed curve resulting in a maximum rate of change of 0.66°/year and a mean 0.10 ± 0.10°/year may be a more realistic representation of the field behavior. No reverse NRMs were observed, but geomagnetic field excursions may be present where the VGPs deviate by more than 40°from the geographic north at about 52 and 41 ka; the latter may represent the Laschamp event.
KW - Lacustrine sediment
KW - Magnetic inclination
KW - Paleomagnetism
KW - Pleistocene
KW - Secular variations
UR - http://www.scopus.com/inward/record.url?scp=0032448937&partnerID=8YFLogxK
U2 - 10.1016/S0012-821X(98)00146-0
DO - 10.1016/S0012-821X(98)00146-0
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AN - SCOPUS:0032448937
SN - 0012-821X
VL - 161
SP - 145
EP - 160
JO - Earth and Planetary Science Letters
JF - Earth and Planetary Science Letters
IS - 1-4
ER -