Single domain grain distributions II. The distribution of single domain iron grains in Apollo 11 lunar dust

Details Single domain grain distributions II. The distribution of single domain iron grains in Apollo 11 lunar dust Single domain grain distributions II. The distribution of single domain iron grains in Apollo 11 lunar dust

Sep 1971

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1971pepi....4..361s&link_type=abstract

Physics of the Earth and Planetary Interiors, Volume 4, Issue 5, p. 361-369.

Physics

13

Scientific paper

A quantitative analysis of some of the magnetic properties of an Apollo 11 lunar dust sample is given. The measurements involved are the acquisition of isothermal and viscous remanence, the thermal demagnetization of isothermal and thermoremanence, and the temperature and frequency dependence of the initial susceptibility. It is shown that the experimental results are in good agreement with those predicted from single domain theory and can be explained on the basis of an assembly of single domain iron grains distributed such that the number of grains within a given volume range is inversely proportional to the square of the volume.

Affiliated with

Also associated with

No associations

Rating

Single domain grain distributions II. The distribution of single domain iron grains in Apollo 11 lunar dust 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 Single domain grain distributions II. The distribution of single domain iron grains in Apollo 11 lunar dust, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Single domain grain distributions II. The distribution of single domain iron grains in Apollo 11 lunar dust will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1378045