Astronomy and Astrophysics – Astronomy
Scientific paper
Apr 1999
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999geoji.137..261t&link_type=abstract
Geophysical Journal International, Volume 137, Issue 1, pp. 261-265.
Astronomy and Astrophysics
Astronomy
6
Arm, Palaeointensity, Trm
Scientific paper
The theoretical background of ARM correction in Shaw's palaeointensity method was examined by a computer simulation. A case study using Jaep's ARM model, which is based on Néel's relaxation theory, was made for an ensemble of single-domain grains of magnetite which have a log-normal grain distribution (d=0.050 rommu m and barH_C=50 mT with a relative standard deviation of 36 per cent). Variations in the capacities of ARM and TRM were calculated when volume or coercivity was changed up to +/- 50 per cent. If the grain interaction effect is ignored in ARM, the change in ARM capacity due to a change in volume is almost identical to that of TRM. For a more realistic case with grain interaction effects in ARM, the change in capacity due to a change in volume is different in ARM and TRM, although the difference is about 6-7 per cent at most for a change of +/- 20 per cent in ARM capacity. When coercivity is changed, the difference is within about 5 per cent for the 20 per cent change in ARM capacity, although the difference is larger when grain interaction is ignored in ARM. It is suggested that ARM correction should be limited to those results in which the ratio of ARM1/ARM2 is moderately close to unity.
No associations
LandOfFree
Theoretical background of ARM correction in the Shaw palaeointensity method 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 Theoretical background of ARM correction in the Shaw palaeointensity method, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Theoretical background of ARM correction in the Shaw palaeointensity method will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1430656