Paleomagnetic field intensity derived from meteorite magnetization

Details Paleomagnetic field intensity derived from meteorite magnetization Paleomagnetic field intensity derived from meteorite magnetization

Jan 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977pepi...13..373n&link_type=abstract

Physics of the Earth and Planetary Interiors, Volume 13, Issue 4, p. 373-379.

Physics

1

Scientific paper

The paleomagnetic field intensity is estimated with the aid of the Koenigsberger-Thellier method for four ordinary chondrites and one carbonaceous chondrite by assuming that the stable NRM component of these meteorites is attributable to the TRM acquired in a low-temperature range (lower than about 400°C) during their extremely-slow cooling process. The results are summarized in Table IV, where the paleomagnetic field intensity ranges from 0.10 to 0.97 Oe. Possible effects of the extremely-slow cooling rate of meteorites and the secondary TRM acquisition of the surface fusion crust upon the original NRM of the meteorite interior are discussed.

Affiliated with

Also associated with

No associations

Rating

Paleomagnetic field intensity derived from meteorite magnetization does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Paleomagnetic field intensity derived from meteorite magnetization, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Paleomagnetic field intensity derived from meteorite magnetization will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-953050